CRUISE REPORT: P17E (Updated JUN 2018) Highlights Cruise Summary Information Section Designation P17E (MR16-09) Expedition designation (ExpoCodes) 49NZ20170208 Chief Scientists Hiroshi Uchida / JAMSTEC Dates 2017 FEB 08 - 2017 MAR 05 Ship Mirai Ports of call Punta Arenas, Chile – Auckland, New Zealand 39° 46.31' S Geographic Boundaries 175° 19.69' W 72° 47.49' W 67° 0.23' S Stations 35 Floats and drifters deployed 3 Argo floats, 2 Deep Argo floats, 5 SOCOM floats, 7 CO2 buoys deployed Moorings deployed or recovered 0 Contact Information: Hiroshi Uchida huchida@jamstec.go.jp Mirai Cruise Report MR16−09 Trans South Pacific Project December 27, 2016 − March 28, 2017 Japan Agency for Marine-Earth Science and Technology (JAMSTEC) Content I. Cruise Information Murata, Harada, Abe and Uchida (JAMSTEC) 1. Cruise ID 2. Name of Vessel 3. Title of Cruise 4. Cruise Period 5. Ports of Departure/call/arrival 6. Research Area 7. Research Map II. Researchers Murata, Harada, Abe and Uchida (JAMSTEC) 1. Chief Scientists 2. Representative of the Science Party and the Proposed Science Plan 3. List of Participants 4. List of Principal Investigator and Person in Charge on the Ship III. Observation 1. Cruise Narrative Murata, Harada, Abe and Uchida (JAMSTEC) 2. Cruise Track and Log Murata, Harada, Abe and Uchida (JAMSTEC) 3. Underway Observation 3.1 Navigation Murata (JAMSTEC), Sueyoshi, Y. Murakami, Tokunaga, Inagaki, Okumura (NME), K. Yoshida, Kimura, M. Murakami (Mirai Crew) 3.2 Swath Bathymetry (MBES, Sub-bottom profiler) Abe (JAMSTEC), Matsumoto (Univ. of Ryukyu), Fujiwara (JAMSTEC), Sueyoshi, Y. Murakami, Tokunaga, Inagaki, Okumura, K. Yoshida (NME), Kimura, M. Murakami (Mirai Crew) 3.3 Three Component and Total Force Magnetometry Abe (JAMSTEC), Matsumoto (Univ. of Ryukyu), Fujiwara (JAMSTEC), Sueyoshi, Y. Murakami, Tokunaga, Inagaki, Okumura, K. Yoshida (NME), Kimura, M. Murakami (NME) 3.4 Sea Surface Gravity Abe (JAMSTEC), Matsumoto (Univ. of Ryukyu), Fujiwara (JAMSTEC), Sueyoshi, Y. Murakami, Tokunaga, Inagaki, Okumura, K. Yoshida (NME), Kimura, M. Murakami (Mirai Crew) 3.5 Surface Meteorological Observations M. Katsumata (JAMSTEC), Sueyoshi, Y. Murakami, Tokunaga, Inagaki, Okumura, K. Yoshida (NME), Kimura, M. Murakami (Mirai Crew) 3.6 Thermo-salinograph and Related Measurements Uchida, Shiozaki, Sasaoka (JAMSTEC), H. Sato, Tamada, Enoki, Kuwahara, Orui (MWJ) 3.7 pCO2 Murata (JAMSTEC), Watai, A. Ono, Deguchi, Fujiki (MWJ) 3.8 Satellite Image Acquisition M. Katsumata (JAMSTEC), Sueyoshi, Y. Murakami, Tokunaga, Inagaki, Okumura, K. Yoshida (NME), Kimura, M. Murakami (Mirai Crew) 3.9 ADCP Kouketsu (JAMSTEC), Schneider (Univ. of Concepcion), Sueyoshi, Y. Murakami, Tokunaga, Inagaki, Okumura, K. Yoshida (NME), Kimura, M. Murakami (Mirai Crew) 3.10 Ceilometer Observation M. Katsumata (JAMSTEC), Sueyoshi, Y. Murakami, Tokunaga, Inagaki, Okumura, K. Yoshida (NME), Kimura, M. Murakami (Mirai Crew) 3.11 Marine Aerosols Noda (Rakuno Gakuen Univ.), Gutierrez (Univ. of Concepcion), O. Yoshida (Rakuno Gakuen Univ.) 3.12 Aerosol Optical Characteristics Measured by Ship-borne Sky Radiometer Aoki (Toyama Univ.), Hayasaka (Tohoku Univ.) 3.13 C-Band Polarimetric Doppler Weather Radar M. Katsumata, Geng (JAMSTEC), Sueyoshi, Y. Murakami, Tokunaga, Inagaki, Okumura, K. Yoshida (NME), Kimura, M. Murakami (Mirai Crew) 3.14 Lidar Observation M. Katsumata, Taniguchi, Geng (JAMSTEC) 3.15 Disdrometers M. Katsumata, Taniguchi, Geng (JAMSTEC) 3.16 GNSS Precipitable Water M. Katsumata, Fujita, Taniguchi (JAMSTEC) 3.17 Ship-borne Measurement of Aerosols Taketani, Kanaya, Miyagawa, Takashima (JAMSTEC), Todo (NIPR), Komazaki (JAMSTEC), Matsui (Nagoya Univ.), Yoshizue (Tokyo Univ. of Sci.) 3.18 Underway CT Murata (JAMSTEC), Watai, A. Ono, Deguchi, Fujiki (MWJ) 3.19 XCTD Uchida (JAMSTEC), Okumura, Inagaki, Kimura (NME), M. Murakami (Mirai Crew) 3.20 Radiosonde Observations M. Katsumata, Geng, Taniguchi (JAMSTEC), Sueyoshi, Y. Murakami (NME) 4. Station Observation 4.1 Single Channel Seismic Survey Abe (JAMSTEC), Nasu, Kuno, Iijima, Hayashi (NME) 4.2 Sediment Core Nagashima (JAMSTEC), Lany (AWI), Arz (IOW), Tokunaga, Inagaki, Y. Murakami (NME), Y. Sato, Hatakeyama, Y. Katayama, Takahashi, Miyajima, Yamaguchi (MWJ) 4.3 Dredge Y. Sato, Hatakeyama, Y. Katayama (MWJ), Abe, Machida (JAMSTEC), Anma (Univ. of Tsukuba), Orihashi (The Univ. of Tokyo) 4.4 Biological Sample Castro (UdeC) 4.5 Suspended Particles Gonzalez, Menshel (IDEAL) 4.6 Physiological Characteristics of Phytoplankton Assemblages in the Southern Patagonia Pacific Margin Waters Iriarte (IDEAL), Shiozaki (JAMSTEC) 4.7 CTDO2 Measurements Uchida (JAMSTEC), Ito, Tanihara, K. Katayama, Oshitani, Kobayashi (MWJ), Sunamura (The Univ. of Tokyo) 4.8 Bottle Salinity Uchida (JAMSTEC), Tanihara, Watanabe (MWJ) 4.9 Oxygen Kumamoto (JAMSTEC), H. Sato, Tamada, Kuwahara, Orui, Htakeyama (MWJ) 4.10 Nutrients Aoyama (JAMSTEC), Sone, A. Ono, Yokogawa, Ishikawa, Y. Sato (MWJ) 4.11 Density Uchida, Shiozaki (JAMSTEC) 4.12 Carbon Items Murata (JAMSTEC), Watai, A. Ono, Deguchi, Fujuki (MWJ) 4.13 Geochemistry and Microbiology: Nitrogen and Carbon Cycles Yoshikawa (JAMSTEC), O. Yoshida, Chida, Iwamatsu, Koya (Rakuno Gakuen Univ.), Makabe (JAMSTEC) 4.14 Vertical Profiles of Microbial Abundance, Activity and Diversity Yokokawa (JAMSTEC), Sunamura (The Univ. of Tokyo), Nunoura (JAMSTEC) 4.15 Chlorophyll a Sasaoka, Shiozaki (JAMSTEC), H. Sato, Enoki, Kuwahara, Tamada, Hatakeyama (MWJ) 4.16 Nitrogen Fixation Shiozaki (JAMSTEC) 4.17 Absorption Coefficients of Particulate Matter and Colored Dissolved Organic Matter (CDOM) Sasaoka (JAMSTEC) 4.18 Calcium E. Ono (JAMSTEC) 4.19 Dissolved Organic Matter and the Associated Parameters Shigemitsu, Yokokawa, Wakita, Murata (JAMSTEC) 4.20 Carbon Isotopes Kumamoto (JAMSTEC) 4.21 Stable Isotopes of Water Uchida, K. Katsumata (JAMSTEC) 4.22 Beryllium Isotopes Kumamoto (JAMSTEC) 4.23 Lowered Acoustic Doppler Current Profiler Kouketsu, Uchida, K. Katsumata (JAMSTEC) 4.24 Micro Rider Kouketsu, Uchida, K. Katsumata (JAMSTEC) 4.25 Sound Velocity Uchida (JAMSTEC), Ito, Tanihara, K. Katayama, Oshitani, Kobayashi (MWJ) 4.26 pH, POC, and HPLC Sampling for SOCCOM Project K. Katsumata, Sasaoka (JAMSTEC), Boss (Univ. of Maine), Dickson, Becker, Talley (SIO), Key (Princeton Univ.) 4.27 Chlorofluorocarbons and Sulfur Hexafluoride Sasaki (JAMSTEC), H. Sato, Hoshino, Orui (MWJ) 5. Floats, Drifters and Moorings 5.1 Argo Floats Masuda, Hosoda, Sato, Hirano (JAMSTEC), Oshitani (MWJ) 5.2 SOCCOM BGC Floats K. Katsumata (JAMSTEC), Riser, Swift (Univ. of Washington), Johnson (MBARI), Boss (Univ. of Maine), Talley (SIO) 5.3 CO2 buoys Murata, Sasaoka (JAMSTEC), Watai, A. Ono, Deguchi, Fujiki (MWJ) I. Cruise Information 1. Cruise ID MR16-09 2. Name of vessel R/V Mirai 3. Title of cruise Trans South Pacific Project 4. Cruise period Leg 1: 27th December 2016 – 17th January 2017 Leg 2: 20th January – 5th February 2017 Leg 3: 8th February – 5th March 2017 Leg 4: 8th March – 28th March 2017 5. Ports of departure/call/arrival Leg 1: Suva, Fuji – Puerto Montt, Chile Leg 2: Puerto Montt, Chile – Punta Arenas, Chile Leg 3: Punta Arenas, Chile – Auckland, New Zealand Leg 4: Auckland, New Zealand – Sekinehama, Japan 6. Research area South Pacific, Chilean coast, Southern Ocean and western North Pacific 7. Research map II. Researchers 1. Chief scientists Leg 1: Akihiko Murata (JAMSTEC) Leg 2: Naomi Harada (JAMSTEC) Leg 3: Hiroshi Uchida (JAMSTEC) Leg 4: Akihiko Murata (JAMSTEC) 2. Representative of the science party and the proposed science plan (1) Naomi Harada, Akihiko Murata and Natsue Abe: (JAMSTEC): Trans Pacific Project: Ocean Acidification, Marine Biodiversity, Pacific Meridional Overturning Circulation, Crustal Evolution; (2) Fumikazu Taketani (JAMSTEC): Ship-borne measurements of aerosols in the marine atmosphere: Investigation of potential influence of marine aerosol particles on the climate; (3) Shuhei Masuda (JAMSTEC): The monitoring of ocean climate change from surface to deep layer in the Southern Ocean by using Argo- type floats; (4) Taichi Yokokawa (JAMSTEC): Geochemical and microbiological processes throughout water column of the Southern Ocean in the eastern Pacific sector; (5) Toshiya Fujiwara (JAMSTEC): Regional distribution of seafloor displacement caused by the 2011 Tohoku-oki earthquake: What happened in the northern Japan Trench? (6) Masaki Katsumata (JAMSTEC): Cumulus-scale air-sea interaction study by shipboard in-situ observations; (7) Chisato Yoshikawa (JAMSTEC): Geochemical and microbiological investigation for sea surface to sea bottom along Chile margin; (8) Kazuma Aoki (Toyama University): Aerosol optical characteristics measured by Ship-borne Sky radiometer; (9) Takeshi Matsumoto (University of the Ryukyus): Cessation of active spreading axes at trenches. 3. List of participants Affili- Name Charge on board ation Occupation ——————————————————— ——————————————————————— ——————— ———————————————— Leg 1: Suva – Puerto Montt Akihiko Murata Chief Scientist JAMSTEC Scientist Masaki Katsumata Meteorology JAMSTEC Scientist Soichiro Sueyoshi Chief Technician/ADCP/ NME Technical Staff Meteorology/Geophysics Yutaro Murakami Meteorology/ADCP/ NME Technical Staff Geophysics Tomonori Watai Chief Technician MWJ Technical Staff CO2-system Properties Sinichiro Yokogawa Nutrients MWJ Technical Staff Hiroyasu Sato DO/TSG MWJ Technical Staff Nagisa Fujiki CO2-system Properties MWJ Technical Staff Leg 2: Puerto Montt – Punta Arenas Naomi Harada Chief Scientist JAMSTEC Scientist Natsue Abe Dredge/Single- JAMSTEC Scientist channel Seismology Kana Nagashima Sediment JAMSTEC Scientist Takuhei Shiozaki CTD/Water Sampling JAMSTEC Scientist Miyako Sato CTD/Water Sampling/ JAMSTEC Technical Staff Sediment Hidetaka Nomaki Sediment JAMSTEC Scientist Chisato Yoshikawa Water Sampling JAMSTEC Scientist Shiki Machida Dredge JAMSTEC Scientist Jun Noda Aerosol/Water sampling RGU Assosiate Professor Shinya Iwasaki Sediment AIST Researcher Kanda Chida Water Sampling RGU Graduate Student Ryo Anma Dredge/Sediment Univ of Lecturer Tsukuba Yuji Orihashi Dredge UT Assistant Professor Frank Lamy Sediment AWI Professor Helge Wolfgang Arz Sediment IOW Professor Leonardo Román Plankton Net UdeC Professor Castro Cifuentes Wolfgang Schneider CTD UdeC Professor Humberto González Water Sampling IDEAL Professor Jose Luis Iriarte FRRF IDEAL Professor Eduardo Menschel A. Water Sampling IDEAL Technical Staff Marcelo Gutiérrez Aerosol/Water Sampling UdeC Researcher Astete Alejandro Jose Sediment UdeC Technical Staff Avila Santis Victor Acuña Sediment/Plankton Net UdeC Technical Staff Wataru Tokunaga Chief Technician/ADCP/ NME Technical Staff Meteorology/Bathymetry/ Geophysics Satsuki Iijima Meteorology/Bathymetry/ NME Technical Staff Geophysics/ADCP Koichi Inagaki Meteorology/Bathymetry/ NME Technical Staff Geophysics/ADCP Yutaro Murakami Meteorology/Bathymetry/ NME Technical Staff Geophysics/ADCP Toshimasa Nasu Single-channel NME Technical Staff Seismology Hiroyuki Hayashi Single-channel NME Technical Staff Seismology Mitsuteru Kuno Single-channel NME Technical Staff Seismology Yusuke Sato Chief Technician/ MWJ Technical Staff Sediment/Dredge Ei Hatakeyama Sediment/Dredge MWJ Technical Staff Yuki Miyajima Sediment/Dredge MWJ Technical Staff Mika Yamaguchi Sediment/Dredge MWJ Technical Staff Yohei Katayama Sediment/Dredge MWJ Technical Staff Kazuma Takahashi Sediment/Dredge MWJ Technical Staff Rei Ito CTD MWJ Technical Staff Sonoka Tanihara Water sampling/Salinity MWJ Technical Staff Atsushi Ono CO2-system Properties MWJ Technical Staff Tomomi Sone Water Sampling/ MWJ Technical Staff Nutrients Haruka Tamada TSG/Water Sampling/DO MWJ Technical Staff Leg 3: Punta Arenas – Auckland Hiroshi Uchida Chief Scientist JAMSTEC Scientist /Density/Isotope of Water/Sound Velocity Yuichiro Kumamoto DO/Water Sampling/ JAMSTEC Scientist Carbon Isotopes/ Beryllium Isotopes Katsuro Katsumata SOCCOM Project/ JAMSTEC Scientist LADCP/Micro Rider Kosei Sasaoka Chlorophyll-a/CDOM/ JAMSTEC Scientist Absorption Coefficient/ CO2 Buoy/SOCCOM Project Etsuro Ono Calcium/Water Sampling/ JAMSTEC Scientist CO2 Buoy Masahito Shigemitsu DOM/Water Sampling JAMSTEC Scientist Kenichi Sasaki CFCs JAMSTEC Scientist Takuma Miyakawa Aerosols JAMSTEC Scientist Taichi Yokokawa Microbiology JAMSTEC Scientist Michinari Sunamura Microbiology UT Assistant Professor Momoka Yoshizue Aerosols TUS Graduate Student Noriko Iwamatsu Geochemistry/ RGU Student Microbiology Minami Koya Geochemistry/ RGU Student Microbiology Shinya Okumura Chief technician/ NME Technical Staff Meteorology/Geophysics/ ADCP/XCTD Koichi Inagaki Meteorology/Geophysics/ NME Technical Staff ADCP/XCTD Ryo Kimura Meteorology/Geophysics/ NME Technical Staff ADCP/XCTD Satoshi Ozawa Chief Technician/ MWJ Technical Staff Water Sampling Kenichi Katayama CTD MWJ Technical Staff Akira Watanabe Water Sampling/Salinity MWJ Technical Staff Shungo Oshitani CTD/Argo MWJ Technical Staff Rio Kobayashi CTD MWJ Technical Staff Shinichiro Yokogawa Nutrients MWJ Technical Staff Tomonori Watai Total Alkalinity/ MWJ Technical Staff Underway DIC Nagisa Fujiki DIC/Underway DIC MWJ Technical Staff Ei Hatakeyama DO/TSG/Chlorophyll-a MWJ Technical Staff Masanori Enoki DO/TSG/Chlorophyll-a MWJ Technical Staff Hironori Sato CFCs MWJ Technical Staff Hiroshi Hoshino CFCs MWJ Technical Staff Misato Kuwahara DO/TSG/Chlorophyll-a MWJ Technical Staff Koki Uda Water Sampling MWJ Technical Staff Yoshiaki Sato Nutrients MWJ Technical Staff Rei Ito CTD/Argo MWJ Technical Staff Sonoka Tanihara Salinity MWJ Technical Staff Atsushi Ono DIC/Underway DIC MWJ Technical Staff Tomomi Sone Nutrients MWJ Technical Staff Haruka Tamada DO/TSG/Chlorophyll-a MWJ Technical Staff Yoshiko Ishikawa Nutrients MWJ Technical Staff Emi Deguchi Total Alkalinity MWJ Technical Staff Masahiro Orui CFCs MWJ Technical Staff Leg 4: Auckland – Sekinehama Akihiko Murata Chief Scientist JAMSTEC Scientist Kazuho Yoshida Chief Technician/ADCP/ NME Technical Staff Meteorology/Geophysics Ryo Kimura Meteorology/ADCP/ NME Technical Staff Geophysics Yoshiko Ishikawa Chief Technician MWJ Technical Staff Masahiro Orui DO/TSG/Chlorophyll-a MWJ Technical Staff Emi Deguchi CO2-system Properties MWJ Technical Staff ------------------------------------------------------------------------- JAMSTEC Japan Agency for Marine-Earth Science and Technology NME Nippon Marine Enterprises, Ltd. MWJ Marine Works Japan, Ltd. RGU Rakuno Gakuen University TUS Tokyo University of Science UdeC University of Conception, Chile IDEAL Centro de Investigación Dinámica de Ecosystemas Marinos de Altas Latitudes, Universidad Austral de Chile SIO Scripps Institution of Oceanography, USA UW University of Washington, USA UT The University of Tokyo AIST National Institute of Advanced Industrial Science and Technology AWI Alfred Wegener Institute, Germany IOW Leibniz-Institute for Baltic Sea Research Warnemünde, Germany 4. List of Principal Investigator and Person in Charge on the Ship The principal investigator (PI) and the person in charge responsible for major parameters measured on the cruise are listed in Table 4.1. Table 4.1. List of principal investigator and person in charge on the ship. ========================================================================= Item Principal Investigator Person in Charge on the Ship ------------------------------------------------------------------------- Underway Navigation Akihiko Murata (JAMSTEC) Souichiro Sueyoshi (NME) (leg 1) murataa@jamstec.go.jp Wataru Tokunaga (NME) (leg 2) Shinya Okumura (NME) (leg 3) Kazuho Yoshida (NME) (leg 4) Bathymetry Natsue Abe (JAMSTEC) Souichiro Sueyoshi (NME) (leg 1) abenatsu@jamstec.go.jp Wataru Tokunaga (NME) (leg 2) Shinya Okumura (NME) (leg 3) Kazuho Yoshida (NME) (leg 4) Magnetic Field Natsue Abe (JAMSTEC) Souichiro Sueyoshi (NME) (leg 1) abenatsu@jamstec.go.jp Wataru Tokunaga (NME) (leg 2) Shinya Okumura (NME) (leg 3) Kazuho Yoshida (NME) (leg 4) Gravity Natsue Abe (JAMSTEC) Souichiro Sueyoshi (NME) (leg 1) abenatsu@jamstec.go.jp Wataru Tokunaga (NME) (leg 2) Shinya Okumura (NME) (leg 3) Kazuho Yoshida (NME) (leg 4) Meteorology Masaki Katsumata (JAMSTEC) Souichiro Sueyoshi (NME) (leg 1) katsu@jamstec.go.jp Wataru Tokunaga (NME) (leg 2) Shinya Okumura (NME) (leg 3) Kazuho Yoshida (NME) (leg 4) TSG Hiroshi Uchida (JAMSTEC) Hironori Sato (MWJ) (leg 1) huchida@jamtec.go.jp Haruka Tamada (MWJ) (leg 2) Masanori Enoki (MWJ) (leg 3) Masahiro Orui (MWJ) (leg 4) pCO2 Akihiko Murata (JAMSTEC) murataa@jamstec.go.jp Tomonori Watai (MWJ) (leg 1) Atsushi Ono (MWJ) (leg 2) Emi Deguchi (MWJ) (legs 3, 4) Underway DIC Akihiko Murata (JAMSTEC) Nagisa Fujiki (MWJ) murataa@jamstec.go.jp ADCP Shinya Kouketsu (JAMSTEC) Souichiro Sueyoshi (NME) (leg 1) skouketsu@jamstec.go.jp Wataru Tokunaga (NME) (leg 2) Shinya Okumura (NME) (leg 3) Kazuho Yoshida (NME) (leg 4) Ceilometer Masaki Katsumata (JAMSTEC) Souichiro Sueyoshi (NME) (leg 1) katsu@jamstec.go.jp Wataru Tokunaga (NME) (leg 2) Shinya Okumura (NME) (leg 3) Kazuho Yoshida (NME) (leg 4) Marine Aerosols Jun Noda (RGU) Jun Noda (RGU) (leg 2) jnoda@rakuno.ac.jp Taichi Yokokawa (JAMSTEC) (leg 3) Sky Radiometer Kazuma Aoki (Univ. of Toyama) none kazuma@sci.u-toyama.ac.jp Doppler Radar Masaki Katsumata (JAMSTEC) Souichiro Sueyoshi (NME) (leg 1) katsu@jamstec.go.jp Wataru Tokunaga (NME) (leg 2) Shinya Okumura (NME) (leg 3) Kazuho Yoshida (NME) (leg 4) Lidar Masaki Katsumata (JAMSTEC) Masaki Katsumata (JAMSTEC) (leg 1) katsu@jamstec.go.jp Disdrometer Masaki Katsumata (JAMSTEC) Masaki Katsumata (JAMSTEC) (leg 1) katsu@jamstec.go.jp GNSS Precipit- Masaki Katsumata (JAMSTEC) Masaki Katsumata (JAMSTEC) (leg 1) able Water katsu@jamstec.go.jp XCTD Hiroshi Uchida (JAMSTEC) Shinya Okumura (NME) huchida@jamstec.go.jp Radiosonde Masaki Katsumata (JAMSTEC) Souichiro Sueyoshi (NME) katsu@jamstec.go.jp Satellite Image Masaki Katsumata (JAMSTEC) Souichiro Sueyoshi (NME) (leg 1) katsu@jamstec.go.jp Wataru Tokunaga (NME) (leg 2) Shinya Okumura (NME) (leg 3) Kazuho Yoshida (NME) (leg 4) MAX-DOAS Hisahiro Takashima (JAMSTEC) Takuma Miyakawa (JAMSTEC) (leg 3) hisahiro@jamstec.go.jp Ozone and CO Yugo Kanaya (JAMSTEC) Takuma Miyakawa (JAMSTEC) (leg 3) yugo@jamstec.go.jp Black Carbon Fumikazu Taketani (JAMSTEC) Takuma Miyakawa (JAMSTEC) (leg 3) Particles taketani@jamstec.go.jp Fluorescent Fumikazu Taketani (JAMSTEC) Takuma Miyakawa (JAMSTEC) (leg 3) Aerosol taketani@jamstec.go.jp Particles Aerosol Takuma Miyakawa (JAMSTEC) Takuma Miyakawa (JAMSTEC) (leg 3) Particle Size miyakawat@jamstec.go.jp Distribution Aerosol Fumikazu Taketani (JAMSTEC) Takuma Miyakawa (JAMSTEC) (leg 3) Particle taketani@jamstec.go.jp Sampling for post-analyses Station Observation Single Channel Natsue Abe (JAMSTEC) Toshimasa Nasu (NME) Seismometer abenatsu@jamstec.go.jp Sediment Core Kana Nagashima (JAMSTEC) Yusuke Sato (MWJ) nagashimak@jamstec.go.jp Dredge Natsue Abe (JAMSTEC) Yusuke Sato (MWJ) abenatsu@jamstec.go.jp Biological Leonardo Román Castro Sample Cifuentes (UdeC) Naomi Harada (JAMSTEC) lecastro@oceanografia.udec.cl Suspended Humberto González (IDEAL) Naomi Harada (JAMSTEC) Particles hgonzale@uach.cl FRRF Jose Luis Iriarte (IDEAL) Naomi Harada (JAMSTEC) jiriarte@uach.cl CTD/O2 Hiroshi Uchida (JAMSTEC) Rei Ito (MWJ) (leg 2) huchida@jamstec.go.jp Kenichi Katayama (MWJ) (leg 3) Salinity Hiroshi Uchida (JAMSTEC) Sonoka Tanihara (MWJ) huchida@jamstec.go.jp Oxygen Yuichiro Kumamoto (JAMSTEC) Hironori Sato (MWJ) (leg 1) kumamoto@jamstec.go.jp Haruka Tamada (MWJ) (legs 2, 3) Masahiro Orui (MWJ) (leg 4) Nutrients Michio Aoyama (Fukushima U.) Tomomi Sone (MWJ) r706@ipc.fukushima-u.ac.jp Density Hiroshi Uchida (JAMSTEC) Takuhei Shiozaki (JAMSTEC) (leg 2) huchida@jamstec.go.jp Hiroshi Uchida (JAMSTEC) (leg 3) CFCs/SF6/N2O Ken’ichi Sasaki (JAMSTEC) Ken’ichi Sasaki (JAMSTEC) ksasaki@jamstec.go.jp DIC Akihiko Murata (JAMSTEC) Atsushi Ono (MWJ) murataa@jamstec.go.jp Alkalinity Akihiko Murata (JAMSTEC) Atsushi Ono (MWJ) (leg 2) murataa@jamstec.go.jp Tomonori Watai (MWJ) (leg 3) Chlorophyll a Kosei Sasaoka (JAMSTEC) Hironori Sato (MWJ) (leg 1) sasaoka@jamstec.go.jp Takuhei Shiozaki (JAMSTEC) (leg 2) Kosei Sasaoka (JAMSTEC) (leg 3) Masahiro Orui (MWJ) (leg 4) CDOM/Absorption Kosei Sasaoka (JAMSTEC) Kosei Sasaoka (JAMSTEC) Coefficients sasaoka@jamstec.go.jp Calcium Etsuro Ono (JAMSTEC) Etsuro Ono (JAMSTEC) onoet@jamstec.go.jp DOM Masahiro Shigemitsu (JAMSTEC) Masahiro Shigemitsu (JAMSTEC) ma-shige@jamstec.go.jp D14C/d13C Yuichiro Kumamoto (JAMSTEC) Yuichiro Kumamoto (JAMSTEC) kumamoto@jamstec.go.jp Beryllium Yuichiro Kumamoto (JAMSTEC) Yuichiro Kumamoto (JAMSTEC) Isotopes kumamoto@jamstec.go.jp d18O/dD Hiroshi Uchida (JAMSTEC) Hiroshi Uchida (JAMSTEC) huchida@jamstec.go.jp N2O/CH4 Osamu Yoshida (RGU) Kanta Chida (RGU) (leg 2) yoshida@rakuno.ac.jp Noriko Iwamatsu (RGU) (leg 3) Cell Abundance Michinari Sunamura (UT) Hidetaka Nomaki (JAMSTEC) (leg 2) sunamura@eps.s.u-tokyo.ac.jp Michinari Sunamura (UT) (leg 3) Microbial Taichi Yokokawa (JAMSTEC) Hidetaka Nomaki (JSMTEC) (leg 2) Diversity taichi.yokokawa@jamstec.go.jp Taichi Yokokawa (JAMSTEC) (leg 3) Microbial Taichi Yokokawa (JAMSTEC) Taichi Yokokawa (JAMSTEC)(leg 3) Carbon Uptake taichi.yokokawa@jamstec.go.jp d13C/CH4 Akiko Makabe (JAMSTEC) Chisato Yoshikawa (JAMSTEC) (leg 2) makabea@jamstec.go.jp Minami Koya (RGU) (leg 3) d15N d18O/N2O Akiko Makabe (JAMSTEC) Chisato Yoshikawa (JAMSTEC) (leg 2) makabea@jamstec.go.jp Noriko Iwamatsu (RGU) (leg 3) d15N d18O/NO3 Chisato Yoshikawa (JAMSTEC) Chisato Yoshikawa (JAMSTEC) (leg 2) yoshikawac@jamstec.go.jp Minami Koya (RGU) (leg 3) d15N/ Chisato Yoshikawa (JAMSTEC) Chisato Yoshikawa (JAMSTEC) (leg 2) chlorophyll yoshikawac@jamstec.go.jp LADCP Shinya Kouketsu (JAMSTEC) Katsuro Katsumata (JAMSTEC) skouketsu@jamstec.go.jp Micro-Rider Shinya Kouketsu (JAMSTEC) Katsuro Katsumata (JAMSTEC) skouketsu@jamstec.go.jp Sound Velocity Hiroshi Uchida (JAMSTEC) Rei Ito (MWJ) (leg 2) huchida@jamstec.go.jp Hiroshi Uchida (JAMSTEC) (leg 3) pH Andrew Dickson (SIO) Katsuro Katsumata (JAMSTEC) adickson@ucsd.edu POC Susan Becker (SIO) Kosei Sasaoka (JAMSTEC) sbecker@ucsd.edu HPLC Susan Becker (SIO) Kosei Sasaoka (JAMSTEC) sbecker@ucsd.edu Floats, Drifters, Moorings ARGO Float Shuhei Masuda (JAMSTEC) Shungo Oshitani (MWJ) smasuda@jamstec.go.jp SOCCOM BGC Stephen Riser (UW) Katsuro Katsumata (JAMSTEC) Float riser@ocean.washington.edu CO2 Buoy Akihiko Murata (JAMSTEC) Akihiko Murata (JAMSTEC) (leg 1) murataa@jamstec.go.jp Kosei Sasaoka (JAMSTEC) (leg 3) JAMSTEC Japan Agency for Marine-Earth Science and Technology NME Nippon Marine Enterprises, Ltd. MWJ Marine Works Japan, Ltd. RGU Rakuno Gakuen University TUS Tokyo University of Science UdeC University of Conception, Chile IDEAL Centro de Investigación Dinámica de Ecosystemas Marinos de Altas Latitudes, Universidad Austral de Chile SIO Scripps Institution of Oceanography, USA UW University of Washington, USA UT The University of Tokyo III. Observation 1. CRUISE NARRATIVE We are now at a transient stage moving from Holocene, which is characterized by a stable climate, to a new era: Anthropocene. Impacts due to human activities upon surface environment of the earth are appearing as catastrophic climate changes and the related collapse of ecosystem. In addition, as demonstrated by a series of great earthquakes occurred off Chilean coast, off Sumatra and off East Japan, and volcanic activities linked to the earthquakes, it can be said that we are now in the era, when the interior of the earth or crust is in an active phase. Therefore, the present cruise was aimed at clarifying what happened, in this Anthropocene, era of great earth changes, in the fields on surface environment of the earth and those in the interior of it, focusing emergent and confronting issues: 1) Changes in heat and material transports by ocean circulation; 2) Detection of progressive ocean acidification and the response of marine biology, and relationship between biodiversity of marine organisms and changes in living environment; 3) Interaction among mantle, ocean ridge, and subduction system. In the cruise, 8 science plans (see II 2) adopted by the Mirai science committee were also conducted together with the main mission: Trans South Pacific Project. 2. CRUISE TRACK AND LOG Cruise tracks and positions at each day are shown in the following figures, separately for respective legs. (see .pdf version) 3. UNDERWAY OBSERVATION 3.1 Navigation (1) Personnel Akihiko Murata JAMSTEC: Principal investigator*1 - leg1,2,3,4 - Souichiro Sueyoshi Nippon Marine Enterprises Ltd., (NME) - leg1 - Yutaro Murakami NME - leg1,2 - Wataru Tokunaga NME - leg2 - Koichi Inagaki NME - leg2,3 - Shinya Okumura NME - leg3 - Kazuho Yoshida NME - leg4 - Ryo Kimura MIRAI crew / NME - leg1,3,4 - Masanori Murakami MIRAI crew - leg2,3,4 - *1 leg1,4: On-board, leg2,3: Not on-board (2) System description Ship’s position and velocity were provided by Navigation System on R/V MIRAI. This system integrates GNSS position, Doppler sonar log speed, Gyro compass heading and other basic data for navigation. This system also distributed ship’s standard time synchronized to GPS time server via Network Time Protocol. These data were logged on the network server as “SOJ” data every 5 seconds. Sensors for navigation data are listed below; i) GNSS system: R/V MIRAI has four GNSS systems, all GNSS positions were offset to radar-mast position, datum point. Anytime changeable manually switched as to GNSS receiving state. a) StarPack-D & Multi-Fix (version 6), Differential GNSS system. Antenna: Located on compass deck, starboard. b) StarPack-D & Multi-Fix (version 6), Differential GNSS system. Antenna: Located on compass deck, portside. c) Standalone GPS system. Receiver: Trimble SPS751 Antenna: Located on navigation deck, starboard. d) Standalone GPS system. Receiver: Trimble SPS751 Antenna: Located on navigation deck, portside. ii) Doppler sonar log: FURUNO DS-30, which use three acoustic beam for current measurement under the hull. iii) Gyro compass: TOKYO KEIKI TG-6000, sperry type mechanical gyrocompass. iv) GPS time server: SEIKO Precision TS-2540 Time Server, synchronizing to GPS satellites every 1 second. (3) Data period (Time in UTC) Leg1: 17:10, 26 Dec. 2016 to 11:00, 17 Jan. 2017 Leg2: 12:00, 20 Jan. 2017 to 13:00, 05 Feb. 2017 Leg3: 13:10, 08 Feb. 2017 to 21:00, 04 Mar. 2017 Leg4: 21:20, 07 Mar. 2017 to 00:00, 28 Mar. 2017 3.2 Swath Bathymetry (MBES, Sub-bottom profiler) (1) Personnel Natsue Abe JAMSTEC: Principal investigator - leg2 - Takeshi Matsumoto Univ. of the Ryukyus: Principal investigator (Not on board) - leg1,2,3,4 - Toshiya Fujiwara JAMSTEC: Principal investigator (Not on board) - leg4 - Souichiro Sueyoshi Nippon Marine Enterprises Ltd., (NME) - leg1 - Yutaro Murakami NME - leg1,2 - Wataru Tokunaga NME - leg2 - Koichi Inagaki NME - leg2,3 - Shinya Okumura NME - leg3 - Kazuho Yoshida NME - leg4 - Ryo Kimura MIRAI crew / NME - leg1,3,4 - Masanori Murakami MIRAI crew - leg2,3,4 - (2) Introduction R/V MIRAI is equipped with a Multi narrow Beam Echo Sounding system (MBES), SEABEAM 3012 (L3 Communications, ELAC Nautik). The objective of MBES is collecting continuous bathymetric data along ship’s track to make a contribution to geological and geophysical investigations and global datasets. Also, R/V MIRAI is equipped with a Sub-Bottom Profiler (SBP), Bathy2010 (SyQwest). The objective of SBP is collecting sub-bottom data along ship’s track. (3) Data Acquisition The “SEABEAM 3012” on R/V MIRAI was used for bathymetry mapping in the MR16-09 Leg1 to Leg4 cruises. To get accurate sound velocity of water column for ray-path correction of acoustic multibeam, we used Surface Sound Velocimeter (SSV) data to get the sea surface sound velocity (at 6.62m), and the deeper depth sound velocity profiles were calculated by temperature and salinity profiles from CTD and XCTD data by the equation in Del Grosso (1974) during these cruises. Table 3.2-1 shows system configuration and performance of SEABEAM 3012. Bathy2010 on R/V MIRAI was used for sub-bottom mapping during the Leg2 cruise. Table 3.2-2 shows system configuration and performance of Bathy2010 system. Table 3.2-1: SEABEAM 3012 system configuration and performance ---------------------------------------------------------------------- Frequency: 12 kHz Transmit beam width: 2.0 degree Transmit power: 4 kW Transmit pulse length: 2 to 20 msec. Receive beam width: 1.6 degree Depth range: 50 to 11,000 m Number of beams: 301 beams Beam spacing: Equi-angle Swath width: 60 to 150 degrees Depth accuracy: < 1 % of water depth (average across the swath) Table 3.2-2 Bathy2010 System configuration and performance ------------------------------------------------------------------------- Frequency: 3.5 KHz (FM sweep) Transmit beam width: 23 degree Transmit pulse length: 0.5 to 50 msec Strata resolution: Up to 8 cm with 300 m of bottom penetration according to bottom type Depth resolution: 0.1 feet, 0.1 m Depth accuracy: ±10 cm to 100 m, ± 0.3% to 6,000 m Sound velocity: 1,500 m/s (fix) (4) Data processing of MBES (leg3) i) Sound velocity correction Bathymetry data were corrected with sound velocity profiles calculated from the nearest CTD or XCTD data in the distance. The equation of Del Grosso (1974) was used for calculating sound velocity. The data correction was carried out using the HIPS software version 9.1.4 (CARIS, Canada) ii) Editing and Gridding Editing for the bathymetry data was carried out using the HIPS. Firstly, the bathymetry data during ship’s turning were basically deleted, and spike noise of swath data was removed. Then the bathymetry data were checked by “BASE surface (resolution: 50 m averaged grid)”. Finally, all accepted data were exported as XYZ ASCII data (longitude [degree], latitude [degree], depth [m]), and converted to 150 m grid data using “nearneighbor” utility of GMT (Generic Mapping Tool) software. Table 3.2-3: Parameters for gridding on “nearneighbor” in GMT ------------------------------------------------------------- Gridding mesh size: 150 m Search radius size: 150 m Minimum number of neighbors for grid: 1 ------------------------------------------------------------- (5) Data Archives These data obtained in this cruise will be submitted to the Data Management Group (DMG) in JAMSTEC, and will be opened to the public via “Data Research System for Whole Cruise Information in JAMSTEC (DARWIN)” in JAMSTEC web site. . (6) Remarks (Time in UTC) i) The following periods, the MBES observations were carried out. Leg1: 18:46, 28 Dec. 2016 to 06:00, 15 Jan. 2017 Leg2: 12:11, 21 Jan. 2017 to 14:17, 21 Jan. 2017 14:32, 21 Jan. 2017 to 00:23, 04 Feb. 2017 Leg3: 21:00, 10 Feb. 2017 to 06:59, 03 Mar. 2017 Leg4: 07:03, 09 Mar. 2017 to 09:59, 10 Mar. 2017 10:00, 15 Mar. 2017 to 08:09, 16 Mar. 2017 01:50, 18 Mar. 2017 to 03:43, 26 Mar. 2017 ii) The following periods, the SBP observations were carried out. Leg2: 12:11, 21 Jan. 2017 to 14:17, 21 Jan. 2017 14:32, 21 Jan. 2017 to 00:23, 04 Feb. 2017 iii) The following periods, data acquisition of MBES was suspended due to system trouble. Leg4: 07:38, 09 Mar. 2017 to 07:47, 09 Mar. 2017 04:02, 25 Mar. 2017 to 04:11, 26 Mar. 2017 3.3 Three Component and Total Force Magnetometry (1) Personnel Natsue Abe JAMSTEC: Principal investigator - leg2 - Takeshi Matsumoto Univ. of the Ryukyus: Principal investigator (Not on board) - leg1, 2, 3, 4 - Toshiya Fujiwara JAMSTEC: Principal investigator (Not on board - leg4 - Souichiro Sueyoshi Nippon Marine Enterprise Ltd., (NME) - leg1 - Yutaro Murakami NME - leg1, 2 - Wataru Tokunaga NME - leg2 - Koichi Inagaki NME - leg2, 3 - Shinya Okumura NME - leg3 - Kazuho Yoshida NME - leg4 - Ryo Kimura MIRAI crew / NME - leg1, 3, 4 - Masanori Murakami MIRAI crew - leg2, 3, 4 - (2) Introduction Measurement of magnetic force on the sea surface is required for the geophysical investigations of marine magnetic anomaly caused by magnetization in the upper crust. We measured geomagnetic vector by using a three-component magnetometer and total magnetic force by using a cesium magnetometer. (3) Instruments and Methods A) Three-component magnetometer A shipboard three-component magnetometer system (Tierra Tecnica SFG1214) is equipped on-board R/V MIRAI. Three-axes flux-gate sensors with ring-cored coils are fixed on the fore mast. Outputs from the sensors are digitized by a 20-bit A/D converter (1 nT/LSB), and sampled at 8 times per second. Ship's heading, pitch, and roll are measured by the Inertial Navigation System (INS) for controlling attitude of a Doppler radar. Ship's position and speed data are taken from LAN every second. The relation between a magnetic-field vector observed on-board, Hob, (in the ship's fixed coordinate system) and the geomagnetic field vector, F, (in the Earth's fixed coordinate system) is expressed as: Hob = A R P Y F + Hp (a) where R, P and Y are the matrices of rotation due to roll, pitch and heading of a ship, respectively. A is a 3 x 3 matrix which represents magnetic susceptibility of the ship, and Hp is a magnetic field vector produced by a permanent magnetic moment of the ship's body. Rearrangement of Eq. (a) makes B Hob + Hbp = R P Y F (b) where = A-1, and Hbp = - Hp. The magnetic field, F, can be obtained by measuring R, P, Y and Hob, if and Hbp are known. Twelve constants in B and Hbp can be determined by measuring variation of Hob with R, P and Y at a place where the geomagnetic field, F, is known. B) Cesium magnetometer We measured the total magnetic force by using a cesium marine magnetometer (G-882, Geometrics Inc.) and recorded by G-882 data logger (Ver.1.0.0, Clovertech Co.). The G-882 magnetometer uses an optically pumped Cesium-vapor atomic resonance system. The sensor fish towed from 450m to 500 m behind the vessel to minimize the effects of the ship's magnetic field. Table 3.3-1 shows system configuration of MIRAI cesium magnetometer system. Table 3.3-1: System configuration of MIRAI cesium magnetometer system ------------------------------------------------------------------------- Dynamic operating range: 20,000 to 100,000 nT Absolute accuracy: < ±2 nT throughout range Setting: Cycle rate; 0.1 sec Sensitivity; 0.001265 nT at a 0.1 second cycle rate Sampling rate; 1 sec (3) Data Archive These data obtained in this cruise will be submitted to the Data Management Group of JAMSTEC, and will be opened to the public via “Data Research System for Whole Cruise Information in JAMSTEC (DARWIN)” in JAMSTEC web site. (4) Remarks (Time in UTC) A) Three component magnetometer i) The following periods, observations were carried out. Leg1: 18:45, 28 Dec. 2016 to 06:14, 15 Jan. 2017 Leg2: 12:11, 21 Jan. 2017 to 14:17, 21 Jan. 2017 14:32, 21 Jan. 2017 to 00:23, 04 Feb. 2017 Leg3: 21:00, 10 Feb. 2017 to 06:59, 03 Mar. 2017 Leg4: 07:03, 09 Mar. 2017 to 09:59, 10 Mar. 2017 10:00, 15 Mar. 2017 to 08:09, 16 Mar. 2017 01:50, 18 Mar. 2017 to 00:00, 28 Mar. 2017 ii) The following periods, we made a “figure-eight” turn (a pair of clockwise and anti-clockwise rotation) for calibration of the ship’s magnetic effect. Leg1: 01:47, 29 Dec. 2016 to 02:08, 29 Dec. 2016 around 26-18N, 174-01W 22:00, 03 Jan. 2017 to 22:22, 03 Jan. 2017 around 43-08S, 145-11W 18:00, 11 Jan. 2017 to 18:24. 11 Jan. 2017 around 48-13S, 95-01W 10:10, 14 Jan. 2017 to 10:42, 14 Jan. 2017 around 45-01S, 80-02W Leg2: 20:29, 21 Jan. 2017 to 21:02, 21 Jan. 2017 around 44-21S, 75-33W 05:35, 31 Jan. 2017 to 05:58, 31 Jan. 2017 around 50-43S, 79-12W Leg3: 21:07, 10 Feb. 2017 to 21:41, 10 Feb. 2017 around 59-10S, 73-18W 00:57, 03 Mar. 2017 to 01:17, 03 Mar. 2017 around 39-46S, 175-20W Leg4: 03:00, 18 Mar. 2017 to 03:21, 18 Mar. 2017 around 11-27N, 155-42E 00:41, 25 Mar. 2017 to 01:09, 25 Mar. 2017 around 38-58N, 144-51E 20:08, 25 Mar. 2017 to 20:39, 25 Mar. 2017 around 39-52N, 143-10E iii) The following period, data were invalid due to trouble of the deck box. Leg3: 10:47, 18 Feb. 2017 to 13:39, 18 Feb. 2017 20:49, 25 Feb. 2017 to 00:32, 26 Feb. 2017 iv) The following period, time stamps were delayed 7 seconds. Leg3: 13:39, 18 Feb. 2017 to 22:04, 18 Feb. 2017 v) The following period, data acquisition was suspended due to maintenance. Leg3: 22:04, 18 Feb. 2017 to 22:05, 18 Feb. 2017 00:32, 26 Feb. 2017 to 00:34, 26 Feb. 2017 B) Cesium magnetometer i) The following periods, observations were carried out. Leg1 (Towing distance from stern; 500m): 01:40, 29 Dec. 2016 to 19:01, 04 Jan. 2017 19:50, 04 Jan. 2017 to 15:30, 01 Jan. 2017 16:54, 07 Jan. 2017 to 15:30, 08 Jan. 2017 16:50, 08 Jan. 2017 to 12:30, 14 Jan. 2017 Leg2 (Towing distance from stern; 450m): 20:20, 21 Jan. 2017 to 07:27, 22 Jan. 2017 13:40, 22 Jan. 2017 to 17:15, 22 Jan. 2017 18:43, 22 Jan. 2017 to 23:33, 22 Jan. 2017 02:50, 23 Jan. 2017 to 11:00, 23 Jan. 2017 03:18, 24 Jan. 2017 to 09:35, 24 Jan. 2017 02:09, 25 Jan. 2017 to 05:17, 25 Jan. 2017 11:21, 25 Jan. 2017 to 08:32, 26 Jan. 2017 20:15, 26 Jan. 2017 to 13:36, 27 Jan. 2017 21:12, 27 Jan. 2017 to 06:32, 28 Jan. 2017 21:14, 28 Jan. 2017 to 11:39, 29 Jan. 2017 16:04, 29 Jan. 2017 to 13:33, 30 Jan. 2017 20:18, 30 Jan. 2017 to 07:00, 31 Jan. 2017 20:07, 31 Jan. 2017 to 06:58, 02 Feb. 2017 13:30, 02 Feb. 2017 to 23:53, 02 Feb. 2017 04:34, 03 Feb. 2017 to 18:17, 03 Feb. 2017 Leg3 (Towing distance from stern; 490m) 19:08, 10 Feb. 2017 to 22:55, 14 Feb. 2017 Leg4 (Towing distance from stern; 490m) 01:50, 18 Mar. 2017 to 06:58, 21 Mar. 2017 07:19, 23 Mar. 2017 to 23:30, 25 Mar. 2017 ii) The following period, total magnetic data were invalid due to low signal strength. Leg2: 23:29, 25 Jan. 2017 19:16, 01 Feb. 2017 19:21, 01 Feb. 2017 20:02, 01 Feb. 2017 3.4 Sea Surface Gravity (1) Personnel Natsue Abe JAMSTEC: Principal investigator - leg2 - Takeshi Matsumoto Univ. of the Ryukyus: - leg1, 2, 3, 4 - Principal investigator (Not on board) Toshiya Fujiwara JAMSTEC: - leg4 - Principal investigator (Not on board) Souichiro Sueyoshi Nippon Marine Enterprises Ltd., (NME) - leg1 - Yutaro Murakami NME - leg1, 2 - Wataru Tokunaga NME - leg2 - Koichi Inagaki NME - leg2, 3 - Shinya Okumura NME - leg3 - Kazuho Yoshida NME - leg4 - Ryo Kimura MIRAI crew / NME - leg1, 3, 4 - Masanori Murakami MIRAI crew - leg2, 3, 4 - (2) Introduction The local gravity is an important parameter in geophysics and geodesy. We collected gravity data at the sea surface. (3) Parameters Relative Gravity [CU: Counter Unit] [mGal] = (coef1: 0.9946) * [CU] QC Filter : 120sec. filtered (4) Data Acquisition We measured relative gravity using LaCoste and Romberg air-sea gravity meter S-116 (Micro-G LaCoste, LLC) in the MR16-09 Leg1 to Leg4 cruises. To convert the relative gravity to absolute one, we measured gravity, using portable gravity meter (CG-5, Scintrex), at Shimizu, Punta Arenas and Sekinehama as the reference points. (5) Preliminary Results Absolute gravity table is shown in Table 3.4-1. Table 3.4-1: Absolute gravity table of the MR16-09 cruise Absolute Sea Ship Gravity at S-116 No. Date UTC Port Gravity Level Draft Sensor * Gravity yy/mm/dd [mGal] [cm] [cm] [mGal] [mGal] --- -------- ----- ---------- ---------- ----- ----- ---------- -------- #1 16/11/25 06:18 Shimizu 979729.626 128 645 979730.18 12014.81 #2 17/03/28 08:35 Sekinehama 980371.862 200 600 980372.63 12685.04 *: Gravity at Sensor = Absolute Gravity + Sea Level*0.3086/100 + (Draft-530)/100*0.2222 (6) Data Archive These data obtained in this cruise will be submitted to the Data Management Group (DMG) in JAMSTEC, and will be opened to the public via “Data Research System for Whole Cruise Information in JAMSTEC (DARWIN)” in JAMSTEC web site. . (7) Remarks (Time in UTC) i) The following periods, the observation were carried out. Leg1: 18:46, 28 Dec. 2016 to 06:13, 15 Jan. 2017 Leg2: 12:11, 21 Jan. 2017 to 14:17, 21 Jan. 2017 14:32, 21 Jan. 2017 to 00:23, 04 Feb. 2017 Leg3: 21:00, 10 Feb. 2017 to 06:59, 03 Mar. 2017 Leg4: 07:03, 09 Mar. 2017 to 09:59, 10 Mar. 2017 10:00, 15 Mar. 2017 to 08:09, 16 Mar. 2017 01:50, 18 Mar. 2017 to 00:00, 28 Mar. 2017 ii) The following period, depth data was available Leg1: 18:47, 28 Dec. 2016 to 05:39, 15 Jan. 2017 Leg2: 12:11, 21 Jan. 2017 to 14:17, 21 Jan. 2017 14:32, 21 Jan. 2017 to 00:23, 04 Feb. 2017 Leg3: 21:00, 10 Feb. 2017 to 06:59, 03 Mar. 2017 Leg4: 07:05, 09 Mar. 2017 to 07:37, 09 Mar. 2017 07:48, 09 Mar. 2017 to 09:59, 10 Mar. 2017 10:00, 15 Mar. 2017 to 08:09, 16 Mar. 2017 01:50, 18 Mar. 2017 to 04:01, 25 Mar. 2017 04:12, 25 Mar. 2017 to 03:43, 26 Mar. 2017 3.5 Surface Meteorological Observations (1) Personnel Masaki Katsumata JAMSTEC: Principal investigator*1 - leg1,2,3,4 - Souichiro Sueyoshi Nippon Marine Enterprise Ltd., (NME) - leg1 - Yutaro Murakami NME - leg1,2 - Wataru Tokunaga NME - leg2 - Koichi Inagaki NME - leg2,3 - Shinya Okumura NME - leg3 - Kazuho Yoshida NME - leg4 - Ryo Kimura MIRAI crew / NME - leg1,3,4 - Masanori Murakami MIRAI crew - leg2,3,4 - *1 leg1:On-board, leg2,3,4:Not on-board (2) Objectives Surface meteorological parameters are observed as a basic dataset of the meteorology. These parameters provide the temporal variation of the meteorological condition surrounding the ship. (3) Methods Surface meteorological parameters were observed from the MR16-09 Leg1 cruise to Leg4 cruise. In these cruises, we used two systems for the observation. i) MIRAI Surface Meteorological observation (SMet) system Instruments of SMet system are listed in Table 3.5-1 and measured parameters are listed in Table 3.5-2. Data were collected and processed by KOAC-7800 weather data processor made by Koshin-Denki, Japan. The data set consists of 6-second averaged data. ii) Shipboard Oceanographic and Atmospheric Radiation (SOAR) measurement system SOAR system designed by BNL (Brookhaven National Laboratory, USA) consists of major five parts. a) Portable Radiation Package (PRP) designed by BNL – short and long wave downward radiation. b) Analog meteorological data sampling with CR1000 logger manufactured by Campbell Inc. Canada – wind, pressure, and rainfall (by a capacitive rain gauge) measurement. c) Digital meteorological data sampling from individual sensors - air temperature, relative humidity and rainfall (by ORG (optical rain gauge)) measurement. d) Photosynthetically Available Radiation (PAR) sensor manufactured by Biospherical Instruments Inc. (USA) - PAR measurement. e) Scientific Computer System (SCS) developed by NOAA (National Oceanic and Atmospheric Administration, USA) – centralized data acquisition and logging of all data sets. SCS recorded PRP, CR1000 data, air temperature and relative humidity data, ORG data. SCS composed Event data (JamMet) from these data and ship’s navigation data every 6 seconds. Instruments and their locations are listed in Table 3.5-3 and measured parameters are listed in Table 3.5-4. For the quality control as post processing, we checked the following sensors, before and after the cruise. i. Young rain gauge (SMet and SOAR) Inspect of the linearity of output value from the rain gauge sensor to change input value by adding fixed quantity of test water. ii. Barometer (SMet and SOAR) Comparison with the portable barometer value, PTB220, VAISALA iii. Thermometer (air temperature and relative humidity) ( SMet and SOAR ) Comparison with the portable thermometer value, HM70, VAISALA (4) Preliminary results Fig. 3.5-1 to Fig. 3.5-3 show the time series of the following parameters; Wind (SOAR) Air temperature (SMet) Relative humidity (SMet) Precipitation (SOAR, ORG) Short/long wave radiation (SOAR) Pressure (SMet) Sea surface temperature (SMet) Significant wave height (SMet) (5) Data archives These data obtained in these cruises will be submitted to the Data Management Group of JAMSTEC, and will be opened to the public via “Data Research System for Whole Cruise Information in JAMSTEC (DARWIN)” in JAMSTEC web site. . (6) Remarks (Times in UTC) i) The following periods, the observation were carried out. Leg1: 18:45, 28 Dec. 2016 to 06:13, 15 Jan. 2017 Leg2: 12:11, 21 Jan. 2017 to 14:17, 21 Jan. 2017 14:32, 21 Jan. 2017 to 00:23, 04 Feb. 2017 Leg3: 21:00, 10 Feb. 2017 to 06:59, 03 Mar. 2017 Leg4: 07:03, 09 Mar. 2017 to 09:59, 10 Mar. 2017 10:00, 15 Mar. 2017 to 08:09, 16 Mar. 2017 01:50, 18 Mar. 2017 to 00:00, 28 Mar. 2017 ii) The following periods, sea surface temperature of SMet data was available. Leg1: 18:45, 28 Dec. 2016 to 06:13, 15 Jan. 2017 Leg2: 12:11, 21 Jan. 2017 to 14:17, 21 Jan. 2017 14:32, 21 Jan. 2017 to 00:23, 04 Feb. 2017 Leg3: 21:00, 10 Feb. 2017 to 06:59, 03 Mar. 2017 Leg4: 07:03, 09 Mar. 2017 to 09:59, 10 Mar. 2017 10:00, 15 Mar. 2017 to 08:09, 16 Mar. 2017 01:50, 18 Mar. 2017 to 05:30, 26 Mar. 2017 iii) The following period, downwelling shortwave radiation amount of SOAR was invalid due to a PSP sensor failure. about 13:00, 02 Jan. 2017 to 16:11, 07 Jan. 2017 iv) PSP senor of PRP was replaced to a spare due to a sensor failure at 06:11, 07 Jan. 2017. v) The following period, FRSR data acquisition was stopped due to a trouble of heater in the FRSR sensor. 08:14, 27 Feb. 2017 to 07:00, 03 Mar. 2017 vi) The following period, FRSR data acquisition was suspended to prevent the shadow-band from freezing. 21:25, 12 Feb. 2017 to 23:28, 22 Feb. 2017 vii) The following periods, downwelling shortwave radiation amount and longwave radiation amount data of SOAR were invalid due to PRP system maintenance. 21:15, 06 Jan. 2017 to 21:51, 06 Jan. 2017 15:55, 07 Jan. 2017 to 16:15, 07 Jan. 2017 viii) The following periods, downwelling shortwave radiation amount and longwave radiation amount data of SOAR were not acquired due to PRP system maintenance. 21:23, 12 Feb. 2017 to 21:24, 12 Feb. 2017 23:24, 22 Feb. 2017 to 23:28, 22 Feb. 2017 07:56, 27 Feb. 2017 to 08:13, 27 Feb. 2017 17:33, 27 Feb. 2017 to 17:50, 27 Feb. 2017 23:22, 27 Feb. 2017 to 23:26, 27 Feb. 2017 ix) The following time, increasing of SMet capacitive rain gauge data were invalid due to transmitting for MF/HF or VHF radio. 21:27, 06 Jan. 2017 20:17, 03 Feb. 2017 20:21, 03 Feb. 2017 23:20, 18 Mar. 2017 15:01, 23 Mar. 2017 15:04, 23 Mar. 2017 x) The following time, increasing of SMet optical rain gauge data were invalid due to maintenance. 02:50, 25 Feb. 2017 20:29, 01 Mar. 2017 20:30, 01 Mar. 2017 06:21, 23 Mar. 2017 Table 3.5-1: Instruments and installation locations of MIRAI Surface Meteorological observation system Sensors Type Manufacturer Location (altitude from surface) ---------------------- --------- ----------------------- ------------------------- Anemometer KE-500 Koshin Denki, Japan Foremast (24 m) Tair/RH HMP155 Vaisala, Finland with 43408 Gill aspirated radiation shield R.M. Young, USA Compass deck (21 m) starboard and portside Thermometer: SST RFN2-0 Koshin Denki, Japan 4th deck (-1m, inlet -5m) Barometer Model-370 Setra System, USA Captain deck (13 m) weather observation room Capacitive rain gauge 50202 R. M. Young, USA Compass deck (19 m) Optical rain gauge ORG-815DS Osi, USA Compass deck (19 m) Radiometer (short wave) MS-802 Eko Seiki, Japan Radar mast (28 m) Radiometer (long wave) MS-202 Eko Seiki, Japan Radar mast (28 m) Wave height meter WM-2 Tsurumi-seiki, Japan Bow (10 m) Stern (8m) Table 3.5-2: Parameters of MIRAI Surface Meteorological observation system Parameter Units Remarks ----------------------------------------- ------ --------------------- 1 Latitude degree 2 Longitude degree 3 Ship’s speed knot MIRAI log DS-30, Furuno 4 Ship’s heading degree MIRAI gyro, TG-6000, TOKYO-KEIKI 5 Relative wind speed m/s 6sec./10min. averaged 6 Relative wind direction degree 6sec./10min. averaged 7 True wind speed m/s 6sec./10min. averaged 8 True wind direction degree 6sec./10min. averaged 9 Barometric pressure hPa adjusted to sea surface level 6sec. averaged 10 Air temperature (starboard side) degC 6sec. averaged 11 Air temperature (port side) degC 6sec. averaged 12 Dewpoint temperature (starboard side) degC 6sec. averaged 13 Dewpoint temperature (port side) degC 6sec. averaged 14 Relative humidity (starboard side) % 6sec. averaged 15 Relative humidity (port side) % 6sec. averaged 16 Sea surface temperature degC 6sec. averaged 17 Rain rate (optical rain gauge) mm/hr hourly accumulation 18 Rain rate (capacitive rain gauge) mm/hr hourly accumulation 19 Down welling shortwave radiation W/m2 6sec. averaged 20 Down welling infra-red radiation W/m2 6sec. averaged 21 Significant wave height (bow) m hourly 22 Significant wave height (aft) m hourly 23 Significant wave period (bow) second hourly 24 Significant wave period (aft) second hourly Table 3.5-3: Instruments and installation locations of SOAR system Sensors (Meteorological) Type Manufacturer Location (altitude from surface) ------------------------ ---------------- --------------- -------------------------------- Anemometer 05106 R.M. Young, USA Foremast (25 m) Barometer PTB210 Vaisala, Finland with 61002 Gill pressure port R.M. Young, USA Foremast (23 m) Capacitive rain gauge 50202 R.M. Young, USA Foremast (24 m) Tair/RH HMP155 Vaisala, Finland with 43408 Gill aspirated radiation shield R.M. Young, USA Foremast (23 m) Optical rain gauge ORG-815DR Osi, USA Foremast (24 m) Sensors (PRP) Type Manufacturer Location (altitude from surface) ------------------------ ---------------- --------------- -------------------------------- Radiometer (short wave) PSP Epply Labs, USA Foremast (25 m) Radiometer (long wave) PIR Epply Labs, USA Foremast (25 m) Fast rotating shadowband radiometer Yankee, USA Foremast (25 m) Sensor (PAR) Type Manufacturer Location (altitude from surface) ------------------------ ---------------- --------------- -------------------------------- PAR sensor PUV-510 Biospherical Instruments Inc., USA Navigation deck (18m) Table 3.5-4 Parameters of SOAR system (JamMet) Parameter Units Remarks ----------------------------------------- -------------- -------------- 1 Latitude degree 2 Longitude degree 3 SOG knot 4 COG degree 5 Relative wind speed m/s 6 Relative wind direction degree 7 Barometric pressure hPa 8 Air temperature degC 9 Relative humidity % 10 Rain rate (optical rain gauge) mm/hr 11 Precipitation (capacitive rain gauge) mm reset at 50 mm 12 Down welling shortwave radiation W/m2 13 Down welling infra-red radiation W/m2 14 Defuse irradiance W/m2 15 PAR microE/cm2/sec Fig. 3.5-1: Time series of surface meteorological parameters during the MR16-09 Leg1 cruise Fig. 3.5-2: Time series of surface meteorological parameters during the MR16-09 Leg3 cruise Fig. 3.5-3: Time series of surface meteorological parameters during the MR16-09 Leg4 cruise 3.6 Thermo-Salinograph and Related Measurements May 17, 2017 (1) Personnel Hiroshi Uchida (JAMSTEC) Takuhei Shiozaki (JAMSTEC) Kosei Sasaoka (JAMSTEC) Hironori Sato (MWJ) Haruka Tamada (MWJ) Masanori Enoki (MWJ) Misato Kuwahara (MWJ) Masahiro Orui (MWJ) (2) Objectives The objective is to collect sea surface salinity, temperature, dissolved oxygen, fluorescence and turbidity data continuously along the cruise track. (3) Materials and methods The Continuous Sea Surface Water Monitoring System (Marine Works Japan Co, Ltd.) has seven sensors and automatically measures salinity, temperature, dissolved oxygen, fluorescence, and turbidity in sea surface water every one minute. This system is located in the sea surface monitoring laboratory and bottom of the ship and connected to shipboard LAN system. Measured data along with time and location of the ship were displayed on a monitor and stored in a desktop computer. The sea surface water was continuously pumped up to the laboratory from about 5 m water depth and flowed into the system through a vinyl-chloride pipe. One thermometer is located just before the sea water pump at bottom of the ship. The flow rate of the surface seawater was controlled to be about 1.2 L/min. Periods of measurement, maintenance and problems are listed in Table 3.6.1. Software and sensors used in this system are listed below. i. Software Seamoni-kun Ver.1.50 ii. Sensors Temperature and conductivity sensor Model: SBE 45, Sea-Bird Electronics, Inc. Serial number: 4557820-0319 Pre-cruise calibration: 19 May 2016, Sea-Bird Electronics, Inc. Bottom of ship thermometer Model: SBE 38, Sea-Bird Electronics, Inc. Serial number: 3852788-0457 Pre-cruise calibration: 8 March 2016, Sea-Bird Electronics, Inc. Dissolved oxygen sensor Model: RINKO-II, JFE Adantech Co. Ltd. Serial number: 0013 Pre-cruise calibration: 24 April 2016, JAMSTEC Model: OPTODE 3835, Aanderaa Data Instruments, AS. Serial number: 1915 Pre-cruise calibration: 13 May 2015, JAMSTEC Fluorometer and turbidity sensor Model: C3, Turner Designs, Inc. Serial number: 2300384 Table 3.6.1: Events of the Continuous Sea Surface Water Monitoring System operation. System Date System Time Event [UTC] [UTC] Leg 1 ———————————————————————————————————————————————————————————————————— 2016/12/28 18:46 Logging start 2017/01/06 00:11~00:57 Logging stop for filter cleaning 2017/01/15 06:12 Logging stop Leg 2 ———————————————————————————————————————————————————————————————————— 2017/01/21 12:11 Logging start 2017/01/21 14:18~14:31 All data unavailable 2017/01/28 11:01~11:43 Logging stop for filter cleaning 2017/01/28 12:02~12:03 C3 data unavailable 2017/01/28 19:14~19:15 All data unavailable 2017/01/28 19:15~19:18 C3 data unavailable 2017/01/28 20:15~21:21 Logging stop for entering into Chilean territorial waters 2017/01/31 08:50~08:55 Flow rate for RINKO/Optode was zero 2017/02/03 23:59 Logging stop Leg 3 ———————————————————————————————————————————————————————————————————— 2017/02/10 21:15 Logging start 2017/02/16 03:17~04:10 Logging stop for filter cleaning 2017/02/16 08:16~15:46 Flow rate for RINKO/Optode might be small 2017/02/16 20:55~ Flow rate for SBE 45 was unstable 2017/02/17 ~12:07 2017/02/17 12:08~13:25 Logging stop for filter cleaning 2017/03/03 07:00 Logging stop Leg 4 ———————————————————————————————————————————————————————————————————— 2017/03/09 07:03 Logging start 2017/03/10 10:00~ Logging stop for entering into foreign EEZs 2017/03/15 ~09:59 2017/03/16 08:10~ Logging stop for entering into foreign EEZs 2017/03/18 ~01:49 2017/03/25 23:00 Logging stop (4) Pre-cruise calibration Pre-cruise sensor calibrations for the SBE 45 and SBE 38 were performed at Sea-Bird Electronics, Inc. Pre-cruise sensor calibrations for the oxygen sensors were performed at JAMSTEC. The oxygen sensors were immersed in fresh water in a 1-L semi-closed glass vessel, which was immersed in a temperature-controlled water bath. Temperature of the water bath was set to 1, 10, 20 and 29ºC. Temperature of the fresh water in the vessel was measured by a thermistor thermometer (expanded uncertainty of smaller than 0.01ºC, ARO-PR, JFE Advantech, Co., Ltd.). At each temperature, the fresh water in the vessel was bubbled with standard gases (4, 10, 17 and 25% oxygen consisted of the oxygen-nitrogen mixture, whose relative expanded uncertainty is 0.5%) for more than 30 minutes to insure saturation. Absolute pressure of the vessel headspace was measured by a reference quartz crystal barometer (expanded uncertainty of 0.01% of reading) and ranged from about 1040 to 1070 hPa. The data were averaged over 5 minutes at each calibration point (a matrix of 24 points). As a reference, oxygen concentration of the fresh water in the calibration vessel was calculated from the oxygen concentration of the gases, temperature and absolute pressure at the water depth (about 8 cm) of the sensor’s sensing foil as follows: O2 (µmol/L) = {1000 × c(T) × (Ap – pH2O)} / {0.20946 × 22.3916 × (1013.25 – pH2O)} where c(T) is the oxygen solubility, Ap is absolute pressure [in hPa], and pH2O is the water vapor pressure [in hPa]. The RINKO was calibrated by the modified Stern-Volmer equation slightly modified from a method by Uchida et al. (2010): O2 ((mol/L) = [(V0 / V)E – 1] / Ksv where V is raw phase difference, V0 is raw phase difference in the absence of oxygen, Ksv is Stern-Volmer constant. The coefficient E corrects nonlinearity of the Stern-Volmer equation. The V0 and the Ksv are assumed to be functions of temperature as follows. Ksv = C0 + C1 × T + C2 × T2 V0 = 1 + C3 × T V = C4 + C5 × Vb where T is CTD temperature (°C) and Vb is raw output. The oxygen concentration is calculated using accurate temperature data from the SBE 45 instead of temperature data from the RINKO. The calibration coefficients were as follows: C0 = 5.123682697760924e–3 C1 = 2.216599487021134e–4 C2 = 4.123214071344090e–6 C3 = –6.672929550710492e–4 C4 = 2.395966849477748e–2 C5 = 0.1951644347447042 E = 1.5 (5) Data processing and post-cruise calibration Data from the Continuous Sea Surface Water Monitoring System were obtained at 1 minute intervals. These data were processed as follows. Spikes in the temperature and salinity data were removed using a median filter with a window of 3 scans (3 minutes) when difference between the original data and the median filtered data was larger than 0.1ºC for temperature and 0.5 for salinity. Data gaps were linearly interpolated when the gap was ≤ 13 minutes. Fluoromete and turbidity data were low- pass filtered using a median filter with a window of 3 scans (3 minutes) to remove spikes. Raw data from the RINKO oxygen sensor, fluorometer and turbidity data were low-pass filtered using a Hamming filter with a window of 15 scans (15 minutes). Salinity (S [PSU]), dissolved oxygen (O [Smol/kg]), and fluorescence (Fl [RFU]) data were corrected using the water sampled data. Details of the measurement methods are described in Sections 4.8, 4.9 and 4.15 for salinity, dissolved oxygen, and chlorophyll-a, respectively. Corrected salinity (Scor), dissolved oxygen (Ocor), and estimated chlorophyll a (Chl-a) were calculated from following equations Scor [PSU] = c0 + c1 S + c2 t Ocor [[mol/kg] = c0 + c1 O + c2 T + c3 t Chl-a [tg/L] = c0 + c1 Fl where S is practical salinity, t is days from a reference time (2016/12/28 18:46 [UTC]), T is temperature in ºC. The best fit sets of calibration coefficients (c0~c3) were determined by a least square technique to minimize the deviation from the water sampled data. The calibration coefficients were listed in Table 3.6.2. Comparisons between the Continuous Sea Surface Water Monitoring System data and water sampled data are shown in Figs. 3.6.1, 3.6.2 and 3.6.3. The calibration coefficients were basically determined for each leg. For leg 3, salinity data were shifted at routine maintenance (2017/02/16 03:17~04:10). Therefore, the coefficient c0 was changed before and after the maintenance. For fluorometer data, water sampled data obtained at night [PAR (Photosynthetically Available Radiation) < 50 = 8) Leg 2 (for ~ 2017/01/25 19:50 or 2017/01/29 19:50 ~) 0.0 6.722433e–2 (for Fl < 7) –0.3219685 0.1132198 (for Fl >= 7) (for 2017/01/25 19:50 ~ 2017/01/29 19:50) 0.0 0.1164691 (for Fl < 8) –3.496350 0.5535129 (for Fl >= 8 and Fl < 12) 2.689773 3.800260e–2 (for Fl >= 12) Leg 3 0.0 5.766692e–2 (for Fl < 8) –0.1513446 7.658499e–2 (for Fl >= 8) Leg 4 0.0 0.1164691 (for Fl < 8) –3.496350 0.5535129 (for Fl >= 8 and Fl < 12) 2.689773 3.800260e–2 (for Fl >= 12) Figure 3.6.1: Comparison between TSG salinity (red: before correction, green: after correction) and sampled salinity. Figure 3.6.2: Comparison between TSG oxygen (red: before correction, green: after correction) and sampled oxygen. Figure 3.6.3: Comparison between TSG fluorescence and sampled chlorophyll-a. Open dots show that PAR data were greater than 50 FE/(m2 sec). Calibration functions are also shown as lines. 3.7 pCO2 (1) Personnel Akihiko Murata (JAMSTEC) Tomonori Watai (MWJ) Atsushi Ono (MWJ) Emi Deguchi (MWJ) Nagisa Fujiki (MWJ) (2) Objective Concentrations of CO2 in the atmosphere are now increasing at a rate of about 2.0 ppmv y–1 owing to human activities such as burning of fossil fuels, deforestation, and cement production. It is an urgent task to estimate as accurately as possible the absorption capacity of the oceans against the increased atmospheric CO2, and to clarify the mechanism of the CO2 absorption, because the magnitude of the anticipated global warming depends on the levels of CO2 in the atmosphere, and because the ocean currently absorbs 1/3 of the 6 Gt of carbon emitted into the atmosphere each year by human activities. In this cruise, we measured pCO2 (partial pressure of CO2) in the atmosphere and surface seawater continuously along cruise tracks in the South Pacific in order to quantify how much CO2 is absorbed in the region. (3) Apparatus Concentrations of CO2 in the atmosphere and the sea surface were measured continuously during the cruise using an automated system with a non-dispersive infrared (NDIR) analyzer (Li-COR LI-7000). The automated system (Nippon ANS) was operated by about one and a half hour cycle. In one cycle, standard gasses, marine air and an air in a headspace of an equilibrator were analyzed subsequently. The nominal concentrations of the standard gas were 230, 290, 370 and 430 ppmv. The standard gases will be calibrated after the cruise. The marine air taken from the bow was introduced into the NDIR by passing through a mass flow controller, which controlled the air flow rate at about 0.6 – 0.8 L/min, a cooling unit, a perma-pure dryer (GL Sciences Inc.) and a desiccant holder containing Mg(ClO4)2. A fixed volume of the marine air taken from the bow was equilibrated with a stream of seawater that flowed at a rate of 4.0 – 5.0 L/min in the equilibrator. The air in the equilibrator was circulated with a pump at 0.7-0.8L/min in a closed loop passing through two cooling units, a perma- pure dryer (GL Science Inc.) and a desiccant holder containing Mg(ClO4)2. (4) Results Concentrations of CO2 (xCO2) of marine air and surface seawater are shown in Fig. 3.7.1, together with SST. Fig. 3.7.1: Preliminary results of concentrations of CO2 (xCO2) in atmosphere (green) and surface seawater (blue), and SST (red) observed during (a) leg 1, (b) leg 3, and (c) leg 4 of MR16-09. 3.8 Satellite Image Acquisition (1) Personnel Masaki Katsumata JAMSTEC: Principal investigator*1 - leg1,2,3,4 - Souichiro Sueyoshi Nippon Marine Enterprise Ltd., (NME) - leg1 - Yutaro Murakami NME - leg1,2 - Wataru Tokunaga NME - leg2 - Koichi Inagaki NME - leg2,3 - Shinya Okumura NME - leg3 - Kazuho Yoshida NME - leg4 - Ryo Kimura MIRAI crew / NME - leg1,3,4 - Masanori Murakami MIRAI crew - leg2,3,4 - *1 leg1: On-board, leg2,3,4: Not on-board (2) Objectives The objectives are to collect cloud data in a high spatial resolution mode from the Advance Very High Resolution Radiometer (AVHRR) on the NOAA and MetOp polar orbiting satellites, and to verify the data from Doppler radar on board. (3) Methods We received the down link High Resolution Picture Transmission (HRPT) signal from satellites, which passed over the area around the R/V MIRAI. We processed the HRPT signal with the in-flight calibration and computed the brightness temperature. A cloud image map around the R/V MIRAI was made from the data for each pass of satellites. We received and processed polar orbiting satellites data from the MR16-09 Leg1 cruise to Leg4 cruise. (4) Data archives These data obtained in these cruises will be submitted to the Data Management Group of JAMSTEC, and will be opened to the public via “Data Research System for Whole Cruise Information in JAMSTEC (DARWIN)” in JAMSTEC web site. . 3.9 ADCP (1) Personnel Shinya Kouketsu JAMSTEC: - leg1,2,3,4 - Principal Investigator(Not on board) Wolfgang Schneider Univ. of Concepcion: - leg2 - Principal Investigator Souichiro Sueyoshi Nippon Marine Enterprises Ltd., (NME) - leg1 - Yutaro Murakami NME - leg1,2 - Wataru Tokunaga NME - leg2 - Koichi Inagaki NME - leg2,3 - Shinya Okumura NME - leg3 - Kazuho Yoshida NME - leg4 - Ryo Kimura MIRAI crew / NME - leg1,3,4 - Masanori Murakami MIRAI crew - leg2,3,4 - (2) Objective To obtain continuous measurement of the current profile along the ship’s track. (3) Methods Upper ocean current measurements were made in the MR16-09 Leg1 to Leg4 cruises, using the hull-mounted Acoustic Doppler Current Profiler (ADCP) system. For most of its operation the instrument was configured for water-tracking mode. Bottom-tracking mode, interleaved bottom-ping with water-ping, was made to get the calibration data for evaluating transducer misalignment angle in the shallow water. The system consists of following components; 1) R/V MIRAI has installed vessel-mount ADCP (acoustic frequency 76.8 kHz “Ocean Surveyor”, Teledyne RD Instruments). It has a phased-array transducer with single ceramic assembly and creates 4 acoustic beams electronically. We mounted the transducer head rotated to a ship- relative angle of 45 degrees azimuth from the keel. 2) For heading source, we use ship’s gyro compass (TOKYO KEIKI, Japan), continuously providing heading to the ADCP system directory. Also we have Inertial Navigation System (PHINS, IXBLUE) which provide high-precision heading and attitude information are stored in “.N2R” data files. 3) Differential GNSS system (Multi-Fix, Fugro, Netherlands) providing precise ship’s position fixes. 4) We used VmDas version 1.46.5 (TRDI) for data acquisition. 5) To synchronize time stamp of pinging with GPS time, the clock of the logging computer is adjusted to GPS time every 8 minutes. 6) The sound speed at the transducer does affect the vertical bin mapping and vertical velocity measurement, is calculated from temperature, salinity (constant value; 35.0 psu) and depth (6.5 m; transducer depth) by equation in Medwin (1975). Data was configured for 8-m intervals starting 23-m below the surface. Every ping was recorded as raw ensemble data (.ENR). Major parameters for the measurement (Direct Command) are shown in Table 3.9-1. (4) Preliminary results Fig.3.9-1 to 3.9-4 show surface current profile along the ship’s track, averaged four depth cells from 6th to 10th, about 55m to 103 m with 30 minutes average. (5) Data archive These data obtained in these cruises will be submitted to the Data Management Group of JAMSTEC, and will be opened to the public via “Data Research System for Whole Cruise Information in JAMSTEC (DARWIN)” in JAMSTEC web site. . (6) Remarks (Time in UTC) i) The following periods, the observations were carried out. Leg1: 18:46, 28 Dec. 2016 to 06:00, 15 Jan. 2017 Leg2: 12:11, 21 Jan. 2017 to 14:174, 21 Feb. 2017 14:32, 21 Jan. 2017 to 00:23, 04 Feb. 2017 Leg3: 21:00, 10 Feb. 2017 to 06:59, 03 Mar. 2017 Leg4: 07:03, 09 Mar. 2017 to 09:59, 10 Mar. 2017 10:00, 15 Mar. 2017 to 08:09, 16 Mar. 2017 01:50, 18 Mar. 2017 to 00:00, 28 Mar. 2017 ii) The following period, Temperature and Sound Velocity data were constant (0.0°C and 1449m/s) due to system trouble. 02:55, 16 Feb. 2017 to 02:19, 19 Feb. 2017 Table 3.9-1: Major parameters Bottom-Track Commands BP = 001 Pings per Ensemble (almost less than 1300m depth) Leg1: None Leg2: 22:19, 21 Jan. 2017 to 06:00, 22 Jan. 2017 21:43, 26 Jan. 2017 to 23:19, 26 Jan. 2017 23:02, 28 Jan. 2017 to 01:25, 29 Jan. 2017 22:55, 03 Feb. 2017 to 23:56, 03 Feb. 2017 Leg3: None Leg4: 07:58, 09 Mar. 2017 to 18:34, 09 Mar. 2017 22:19, 25 Mar. 2017 to 00:00, 28 Mar. 2017 Environmental Sensor Commands EA = +04500 Heading Alignment (1/100 deg) EB = +00000 Heading Bias (1/100 deg) ED = 00065 Transducer Depth (0 - 65535 dm) EF = +001 Pitch/Roll Divisor/Multiplier (pos/neg) [1/99 - 99] EH = 00000 Heading (1/100 deg) ES = 35 Salinity (0-40 pp thousand) EX = 00000 Coord Transform (Xform:Type; Tilts; 3Bm; Map) EZ = 10200010 Sensor Source (C; D; H; P; R; S; T; U) C (1): Sound velocity calculates using ED, ES, ET (temp.) D (0): Manual ED H (2): External synchro P (0), R (0): Manual EP, ER (0 degree) S (0): Manual ES T (1): Internal transducer sensor U (0): Manual EU Timing Commands TE = 00:00:02.00 Time per Ensemble (hrs:min:sec.sec/100) TP = 00:02.00 Time per Ping (min:sec.sec/100) Water-Track Commands WA = 255 False Target Threshold (Max) (0-255 count) WB = 1 Mode 1 Bandwidth Control (0=Wid, 1=Med, 2=Nar) WC = 120 Low Correlation Threshold (0-255) WD = 111 100 000 Data Out (V; C; A; PG; St; Vsum; Vsum^2;#G;P0) WE = 1000 Error Velocity Threshold (0-5000 mm/s) WF = 0800 Blank After Transmit (cm) WG = 001 Percent Good Minimum (0-100%) WI = 0 Clip Data Past Bottom (0 = OFF, 1 = ON) WJ = 1 Rcvr Gain Select (0 = Low, 1 = High) WM = 1 Profiling Mode (1-8) WN = 100 Number of depth cells (1-128) WP = 00001 Pings per Ensemble (0-16384) WS= 0800 Depth Cell Size (cm) WT = 000 Transmit Length (cm) [0 = Bin Length] WV = 0390 Mode 1 Ambiguity Velocity (cm/s radial) Fig 3.9-1: Current profile along the ship’s track, about 55m to 103m depth, averaged every 30 minutes (Leg1). Fig 3.9-2: Current profile along the ship’s track, about 55m to 103m depth, averaged every 30 minutes (Leg2). Fig 3.9-3: Current profile along the ship’s track, about 55m to 103m depth, averaged every 30 minutes (Leg3). Fig 3.9-4: Current profile along the ship’s track, about 55m to 103m depth, averaged every 30 minutes (Leg4). 3.10 Ceilometer observation (1) Personnel Masaki Katsumata JAMSTEC: Principal investigator*1 - leg1,2,3,4 - Souichiro Sueyoshi Nippon Marine Enterprise Ltd., (NME) - leg1 - Yutaro Murakami NME - leg1,2 - Wataru Tokunaga NME - leg2 - Koichi Inagaki NME - leg2,3 - Shinya Okumura NME - leg3 - Kazuho Yoshida NME - leg4 - Ryo Kimura MIRAI crew / NME - leg1,3,4 - Masanori Murakami MIRAI crew - leg2,3,4 - *1 leg1: On-board, leg2,3,4: Not on-board (2) Objectives The information of cloud base height and the liquid water amount around cloud base is important to understand the process on formation of the cloud. As one of the methods to measure them, the ceilometer observation was carried out. (3) Parameters 1. Cloud base height [m]. 2. Backscatter profile, sensitivity and range normalized at 10 m resolution. 3. Estimated cloud amount [oktas] and height [m]; Sky Condition Algorithm. (4) Methods We measured cloud base height and backscatter profile using ceilometer (CL51, VAISALA, Finland). Major parameters for the measurement configuration are shown in Table 3.10-1; Table 3.10-1: Major parameters Laser source: Indium Gallium Arsenide (InGaAs) Diode Transmitting center wavelength: 910±10 nm at 25 degC Transmitting average power: 19.5 mW Repetition rate: 6.5 kHz Detector: Silicon avalanche photodiode (APD) Responsibility at 905 nm: 65 A/W Cloud detection range: 0 ~ 13 km Measurement range: 0 ~ 15 km Resolution: 10 meter in full range Sampling rate: 36 sec Sky Condition: Cloudiness in octas (0 ~ 9) (0:Sky Clear, 1:Few, 3:Scattered, 5-7:Broken, 8:Overcast, 9:Vertical Visibility) On the archive dataset, cloud base height and backscatter profile are recorded with the resolution of 10 m (33 ft). (5) Preliminary results Fig.3.10-1 to Fig.3.10-3 show the time series of 1st, 2nd and 3rd lowest cloud base height during these cruises. (6) Data archives These data obtained in these cruises will be submitted to the Data Management Group of JAMSTEC, and will be opened to the public via “Data Research System for Whole Cruise Information in JAMSTEC (DARWIN)” in JAMSTEC web site. . (7) Remarks (Times in UTC) i) The following periods, the observation were carried out. Leg1: 18:45, 28 Dec. 2016 to 06:13, 15 Jan. 2017 Leg2: 12:11, 21 Jan. 2017 to 14:174, 21 Feb. 2017 14:32, 21 Jan. 2017 to 00:23, 04 Feb. 2017 Leg3: 21:00, 10 Feb. 2017 to 06:59, 03 Mar. 2017 Leg4: 07:03, 09 Mar. 2017 to 09:59, 10 Mar. 2017 10:00, 15 Mar. 2017 to 08:09, 16 Mar. 2017 01:50, 18 Mar. 2017 to 00:00, 28 Mar. 2017 ii) The following time, the window was cleaned. Leg1: 04:58, 29 Dec. 2016 01:55, 04 Jan. 2017 21:03, 11 Jan. 2017 Leg2: 11:51, 27 Jan. 2017 00:57, 03 Feb. 2017 Leg3: 01:18, 14 Feb. 2017 22:13, 21 Feb. 2017 02:48, 25 Feb. 2017 20:26, 01 Mar. 2017 Leg4: 02:12, 15 Mar. 2017 06:21, 23 Mar. 2017 Fig. 3.10-1: 1st, 2nd and 3rd lowest cloud base height during MR16-09 Leg1 cruise. Fig. 3.10-2: 1st, 2nd and 3rd lowest cloud base height during MR16-09 Leg3 cruise. Fig. 3.10-3: 1st, 2nd and 3rd lowest cloud base height during MR16-09 Leg4 cruise. 3.11 Marine Aerosols (1) Personnel Jun Noda Rakuno Gakuen University - on board Marcelo Gutiérrez University of Concepcion - on board Osamu Yoshida Rakuno Gakuen University - not on board (2) Objectives • To investigate chemical and biological properties of aerosols in a marine environment • To investigate micron-size particles number and size distribution • To investigate a biological linkage between marine aerosol and seawater (3) Parameters • Chemical and biological compositions of marine aerosols • Particle number concentration • Comparison of biological diversities in ocean water and marine aerosols (4) Instruments and methods (4-1) Marine aerosol collection (4-1-1) Aerosol collection with NILU filter unit with NL PM2.5 cut off impactor The NILU (Norwegian Institute for Air Research, Norway) 2-stage filter holder unit with NL PM2.5 impactor (Tokyo Dylec, Japan) was equipped with two PTFE (Polytetrafluoroethylene) membrane filters with pore size of 0.8 µm (Top:e=47 with 20 mm hole in the center and Bottom:=47mm) to collect two size ranges of marine aerosols. The sampling unit was mounted on the roof section of navigation deck close to a high volume sampler. The Filter units withdraw 4L/min. by a vacuum pump and a Mass Flow Controller (MFC) to maintain the flow rate. Also, the MFC counted the total volume of air passed through the filter unit. The sampling intervals were ca. 24 hr during the leg 2. and ca. 24 hr to 7.8 days during the leg 3 (detail information are shown on the Table 3.11-1 and 3.11-2 Logs of marine aerosol sampling on PTFE membrane filters). (4-2) BioSampler The BioSampler (SKC, USA) was employed to collect marine aerosols from the right side of the upper deck. The BioSampler has three critical orifice nozzles with designated flow direction to create a vortex inside the collection liquid of 15 ml. Also the nozzles act as critical orifice to maintain the flow rate through the nozzle at ca. 10 L/min. At initial trial, sampling duration was ca. 30 min during the surface water sampling period, which was strictly limited to this period to minimize the workload for the ship crews. The Biosampler has a greater capacity to collect biological aerosols than the NILU filter method; we expect to have much more DNA and other biogenic substances in the collection liquid. After the initial trial, there was a discussion about possible prolonged sampling period to ensure more than adequate amount of DNA with onboard Chilean Scientists. After the consultation with the chief scientist and the Chilean side chief scientist, we have decided to conduct sampling of marine aerosols with increased amount of collection liquid and prolonged sampling duration (detail information are shown in the Table 3.11-3. Logs of marine aerosol sampling with BioSampler). (4-3) Particle number concentration and size distribution The particle number concentration and size distributions were planned to measure with Optical Particle Sizer (OPS3330). However, the instrument was not functioning during the leg 2, thus none of the data sets was obtained by the OPS 3330. (5) Station list or Observation log Table 3.11-1: Log of marine aerosol sampling on PTFE membrane filters Date Collected Latitude Longitude On board ID ——————————————————————————————— —————————————————— ————————————————— yyyy MM DD hh:mm:ss UTC/JST Deg. Min. N/S Deg. Min. E/W —————————————— ———— —— —— ———————— ——————— ———— ——————— ——— ———— ——————— ——— MR1609-Tel-001 2017 01 21 13:35 UTC 44 17.3760 S 75 35.4831 W MR1609-Tel-002 2017 01 22 13:35 UTC 46 03.9138 S 75 41.4622 W 2017 01 22 13:40 UTC 46 03.5267 S 75 41.4220 W MR1609-Tel-003 2017 01 23 13:40 UTC 46 04.2428 S 76 32.01270 W 2017 01 23 13:45 UTC 46 04.2314 S 76 32.06210 W MR1609-Tel-004 2017 01 24 13:35 UTC 46 10.7887 S 76 17.68200 W 2017 01 24 13:38 UTC 46 10.7960 S 76 17.67470 W MR1609-Tel-005 2017 01 25 13:37 UTC 46 17.7684 S 76 49.21520 W 2017 01 25 13:41 UTC 46 17.9294 S 76 49.97760 W MR1609-Tel-006 2017 01 26 13:40 UTC 47 46.0578 S 76 24.98860 W 2017 01 26 13:43 UTC 47 46.0370 S 76 24.93060 W MR1609-Tel-007 2017 01 27 13:38 UTC 46 29.5537 S 77 17.37910 W 2017 01 27 13:46 UTC 46 29.1496 S 77 17.35700 W MR1609-Tel-008 2017 01 28 13:42 UTC 47 47.6478 S 76 02.48930 W 2017 01 28 13:45 UTC 47 47.7123 S 76 02.57160 W MR1609-Tel-009 2017 01 29 13:52 UTC 48 23.2475 S 76 28.13850 W 2017 01 29 13:55 UTC 48 23.2536 S 76 28.16440 W MR1609-Tel-010 2017 01 30 13:50 UTC 50 49.0803 S 79 00.68380 W 2017 01 30 13:54 UTC 50 48.8939 S 79 01.44170 W MR1609-Tel-011 2017 01 31 13:45 UTC 50 48.3214 S 79 07.15040 W 2017 01 31 13:49 UTC 50 48.3250 S 79 07.16240 W MR1609-Tel-012 2017 02 01 13:49 UTC 53 16.2706 S 76 12.13750 W 2017 02 01 13:55 UTC 53 17.2478 S 76 10.76840 W MR1609-Tel-013 2017 02 02 13:48 UTC 54 20.4553 S 74 39.49880 W 2017 02 02 13:50 UTC 54 20.1487 S 74 39.83210 W 2017 02 03 19:48 UTC 52 19.0665 S 75 56.76900 W Table 3.11-2: Logs of marine aerosol sampling on PTFE membrane filters Date Collected Latitude Longitude On board ID ——————————————————————————————— —————————————————— ————————————————— yyyy MM DD hh:mm:ss UTC/JST Deg. Min. N/S Deg. Min. E/W —————————————— ———— —— —— ———————— ——————— ———— ——————— ——— ———— ——————— ——— MR1609-Tel-022 2017 02 11 19:39 UTC 61 45.6669 S 80 24.0890 W MR1609-Tel-023 2017 02 16 0:03 UTC 66 55.9992 S 125 14.9269 W 2017 02 16 0:03 UTC 66 55.9992 S 125 14.9269 W MR1609-Tel-024 2017 02 17 0:04 UTC 65 38.8478 S 125 57.4883 W 2017 02 17 0:04 UTC 65 38.8478 S 125 57.4883 W MR1609-Tel-025 2017 02 17 23:57 UTC 63 11.8680 S 126 00.6343 W 2017 02 17 23:57 UTC 63 11.8680 S 126 00.6343 W MR1609-Tel-026 2017 02 18 23:53 UTC 62 20.3533 S 126 06.4242 W 2017 02 18 23:53 UTC 62 20.3533 S 126 06.4242 W MR1609-Tel-027 2017 02 20 0:06 UTC 60 00.8449 S 125 58.5689 W 2017 02 20 0:06 UTC 60 00.8449 S 125 58.5689 W MR1609-Tel-028 2017 02 20 23:53 UTC 57 49.5030 S 125 59.9270 W 2017 02 20 23:53 UTC 57 49.5030 S 125 59.9270 W MR1609-Tel-029 2017 02 22 0:21 UTC 55 01.0794 S 125 58.5795 W 2017 02 22 0:21 UTC 55 01.0794 S 125 58.5795 W MR1609-Tel-030 2017 02 23 0:00 UTC 53 01.1720 S 126 00.1355 W 2017 02 23 0:00 UTC 53 01.1720 S 126 00.1355 W 2017 03 02 18:36 UTC Table 3.11-3: Logs of marine aerosol sampling with BioSampler Date Collected Latitude Longitude On board ID ——————————————————————————————— —————————————————— ————————————————— yyyy MM DD hh:mm:ss UTC/JST Deg. Min. N/S Deg. Min. E/W —————————————— ———— —— —— ———————— ——————— ———— ——————— ——— ———— ——————— ——— MR1609-Tel-014 2017 01 24 1:23 UTC 46 10.1910 S 76 17.28530 W MR1609-Tel-015 2017 01 24 1:53 UTC 46 10.1935 S 76 17.28690 W 2017 01 24 1:55 UTC 46 10.1935 S 76 17.28690 W MR1609-Tel-016 2017 01 24 2:15 UTC 46 10.1948 S 76 17.28910 W 2017 01 26 3:10 UTC 47 49.3219 S 76 36.35760 W MR1609-Tel-017 2017 01 26 7:36 UTC 47 45.9932 S 76 12.48200 W 2017 01 27 20:00 UTC 46 24.8541 S 77 18.93600 W MR1609-Tel-018 2017 01 28 14:55 UTC 47 47.9249 S 76 02.09790 W 2017 01 28 22:23 UTC 47 57.3677 S 76 01.44350 W MR1609-Tel-019 2017 01 29 14:55 UTC 48 23.8232 S 76 28.78540 W 2017 01 30 14:15 UTC 50 48.5986 S 79 04.32910 W MR1609-Tel-020 2017 01 31 12:52 UTC 50 48.3102 S 79 06.99480 W 2017 01 31 19:00 UTC 50 48.3240 S 79 07.17860 W MR1609-Tel-021 2017 02 02 10:14 UTC 54 20.1017 S 74 38.17960 W 2017 02 02 18:43 UTC 53 46.4482 S 74 32.70620 W 2017 02 03 19:59 UTC 52 19.0874 S 75 56.70720 W (6) Plan of analyses (6-1) Chemical analysis In marine aerosols, the amount of organic fraction has clear dependency with the abundance of chlorophyll concentrations (O’Dowd et al., 2004). There have been several efforts to use different saccharides and other organic components as a tracer to link the primary production in seawater (Russel et al., 2010, Miyazaki et al., 2016). In this investigation, we would like to analyze the series of saccharides and fatty acids and some inorganic salts to characterize the marine aerosols from the southern Pacific Ocean. (6-2) Biological analysis A contribution of marine biological materials on the surface layer has gained much of attention because of the effective ice-nucleating properties (Wilson et al., 2015). From the field and laboratory measurements, Wilson et al., proposed the components from diatom such as Thalassiosira psudonana may start the ice nucleation at higher temperature than homogenous nucleation of water at much lower temperature of – 48.3 °C (Willson, et al., 2015, Speedy and Angell, 1976). Thus, understanding the biological components such as plankton in marine flora and marine aerosol is important. For the marine aerosol analysis, the collected particulate matters on the Teflon filters will be extracted and analyzed for microbe diversity by metagenomic analysis. Polymerase chain reaction (PCR) amplification to prepare template DNA for pyrosequencing will be carried out. A data analysis will be performed on each read sequence using previously developed computational tools with some modifications (Nakamura et al., 2008, 2009). In order to have comprehensive metagenomics analyses scheme for marine aerosols and seawater, the analysis method found in Nunoura et al. (2015) will also be taken into consideration. (6-3) Biological analysis by Chilean scientist The Chilean scientist plans to extract and quantify DNA from filters containing suspended material collected by BioSampler. Template DNA will be subjected to PCR amplification using general primers to study fungal diversity. If the outcome of these steps will be successful, a further step to do a molecular fingerprint analysis (DGGE, Denaturing Gradient Gel Electrophoresis) will be carried out to compare biological communities collected from BioSampler and surface seawaters. Finally, a deep taxonomic analysis of fungal communities will be performed according to DGGE results. (7) Expected outcome From this investigation, we expect to get some understanding of the linkage between microbial flora in seawater and marine aerosols. The previous studies by Russel et al. (2010) and Wilson et al. (2015) clearly indicated that chemical substances produced by the marine flora including plankton might play a particular role to attribute the type of marine aerosols. This kind of an integrated approach helps to understand the mechanism to derive marine aerosols such as ice nuclei formation and lifetime of the cloud. (8) Data archives These data obtained in this cruise will be submitted to the Data Management Group of JAMSTEC, and will be opened to the public via “Data Research System for Whole Cruise Information in JAMSTEC (DARWIN)” in JAMSTEC web site. References Miyazaki, Y. Coburn, S. Ono, K. T.Ho, T. Pierce, R.B. Kawamura, K., and Volkamer, R. 2016. Contribution of dissolved organic matter to submicron water-soluble organic aerosols in the marine boundary layer over the eastern equatorial Pacific. Atmos. Chem. Phys., 16, 7695- 7707. Nakamura, S. Maeda, N. Miron, I.M. Yoh, M. Izutsu, K. Kataoka, C. Honda, T. Yasunaga, T. Nakaya, T. Kawai, J. Hayashizaki, Y. Horii, T. and Iida, T. 2008. Metagenomic diagnosis of bacterial infections, Emerg. Infect. Dis., 14(11):1784-86. Nakamura, S. Yang, C.S. Sakon, N. Ueda, M. Tougan, T. Yamashita, A. Goto, N. Takahashi, K. Yasunaga, T. Ikuta, K. Mizutani, T. Okamoto, Y. Tagami, M. Morita, R. Maeda, N. Kawai, J. Hayashizaki, Y. Nagai, Y. Horii, T. Iida, T. and Nakaya, T. 2009. Direct metagenomic detection of viral pathogens in nasal and fecal specimens using an unbiased high-throughput sequencing approach, PLoS One. 4(1): e4219. Nunoura, T. Takaki, Y. Hirai, M. Shimamura, S. Makabe, A. Koide, O. Kikuchi, T. Miyazaki, J. Koba, K. Yoshida, N. Sunamura, M. and Takai K. 2015. Hadal biosphere: insight into the microbial ecosystem in the deepest ocean on Earth. Proc. Natl. Acad. Sci. U.S.A., 112(11):1230-1236. O'Dowd. C.D. Facchini, M.C. Cavalli, F. Ceburnis, D. Mircea, M. Decesari, S. Fuzzi, S. Yoon Y.J. and Putaud, J.P. 2004. Biogenically driven organic contribution to marine aerosol. Nature, 431, 676-680. Russell, L.M. Hawkins, L.N. Frossard, A.A. Quinn, P.K. and Bates, T.S. 2010. Carbohydrate-like composition of submicron atmospheric particles and their production from ocean bubble bursting. Proc. Natl. Acad. Sci. U.S.A., 107(15):6652-6657. Wilson, T.W. Ladino, L.A. Alpert, P.A. Breckels, M.N. Brooks, I.M. Browse, J. Burrows, S.M. Carslaw, K.S. Huffman, J.A. Judd, C., Kilthau, W.P. Mason, R.H. McFiggans, G. Miller, L.A. Nájera, J.J. Polishchuk, E. Rae, S. Schiller, C.L. Si, M. Temprado, J.V. Whale, T.F. Wong, J.P. Wurl, O. Yakobi-Hancock, J.D. Abbatt, J.P. Aller, J.Y. Bertram, A.K. Knopf, D.A. and Murray, B.J. 2015. A marine biogenic source of atmospheric ice-nucleating particles. Nature, 525(7568):234-8. Speedy, R.J. and Angell, C.A. 1976. Isothermal compressibility of supercooled water and evidence for a thermodynamic singularity at - 45°C. Journal of Chemical Physics, 65 (3), pp. 851-858. 3.12 Aerosol optical characteristics measured by ship-borne sky radiometer (1) Personnel Kazuma Aoki (University of Toyama) Principal Investigator/ not onboard Tadahiro Hayasaka (Tohoku University) Co-worker / not onboard Sky radiometer operation was supported by Nippon Marine Enterprises, Ltd. (2) Objective Objective of this observation is to study distribution and optical characteristics of marine aerosols by using a ship-borne sky radiometer (POM-01 MK-III: PREDE Co. Ltd., Japan). Furthermore, collections of the data for calibration and validation to the remote sensing data were performed simultaneously. (3) Parameters - Aerosol optical thickness at five wavelengths (400, 500, 675, 870 and 1020 nm) - Ångström exponent - Single scattering albedo at five wavelengths - Size distribution of volume (0.01 µm – 20 µm) - # GPS provides the position with longitude and latitude and heading direction of the vessel, and azimuth and elevation angle of the sun. Horizon sensor provides rolling and pitching angles. (4) Instruments and Methods The sky radiometer measures the direct solar irradiance and the solar aureole radiance distribution with seven interference filters (0.315, 0.4, 0.5, 0.675, 0.87, 0.94, and 1.02 µm). Analysis of these data was performed by SKYRAD.pack version 4.2 developed by Nakajima et al. 1996. (5) Data archives Aerosol optical data are to be archived at University of Toyama (K.Aoki, SKYNET/SKY: http://skyrad.sci.u-toyama.ac.jp/) after the quality check and will be submitted to JAMSTEC. 3.13 C-band polarimetric Doppler weather radar (1) Personnel Masaki KATSUMATA (JAMSTEC) Principal Investigator (onboard Leg-1, not on board Leg-2, 3, 4) Biao GENG (JAMSTEC) (not on board) Soichiro SUEYOSHI (NME) (Leg-1) Yutaro MURAKAMI (NME) (Leg-1, 2) Wataru TOKUNAGA (NME) (Leg-2) Koichi INAGAKI (NME) (Leg-2, 3) Shinya OKUMURA (NME) (Leg-3) Kazuho YOSHIDA (NME) (Leg-4) Ryo KIMURA (NME) (Leg-3, 4) Ryo KIMURA (Mirai Crew) (Leg-1) Masanori MURAKAMI (Mirai Crew) (Leg-2, 3, 4) (2) Objective The objective of the radar observations in this cruise is to investigate structure and evolution of precipitating systems over the globe, especially those related to the south pacific convergence zone (SPCZ) and stratiform clouds over the Southern Ocean. (3) Radar specifications The C-band polarimetric weather Doppler radar on board the R/V Mirai is used. Basic specifications of the radar are as follows: Frequency: 5370 MHz (C-band) Polarimetry: Horizontal and vertical (simultaneously transmitted and received) Transmitter: Solid-state transmitter Pulse Configuration: Using pulse-compression Output Power: 6 kW (H) + 6 kW (V) Antenna Diameter: 4 meter Beam Width: 1.0 degrees INU (Inertial Navigation Unit):PHINS (IXBLUE S.A.S.) (4) Available variables Radar variables, which are converted from the power and phase of the backscattered signal at vertically- and horizontally-polarized channels, are as follows: Radar reflectivity: Z Doppler velocity: Vr Spectrum width of Doppler velocity: SW Differential reflectivity: ZDR Differential propagation phase: ΦDP Specific differential phase: KDP Co-polar correlation coefficients: ρHV (5) Operational methodology The antenna is controlled to point the commanded ground-relative direction, by controlling the azimuth and elevation to cancel the ship attitude (roll, pitch and yaw) detected by the INU. The Doppler velocity is also corrected by subtracting the ship movement in beam direction. For the maintenance, internal signals of the radar are checked and calibrated at the beginning and the end of the cruise. Meanwhile, the following parameters are checked daily; (1) frequency, (2) peak output power, (3) pulse width, and (4) PRF (pulse repetition frequency). The operational mode of the radar during the cruise is shown in Tables 3.13-1. A dual PRF mode is used for a volume scan. For a RHI, vertical point, and surveillance PPI scans, a single PRF mode is used. (6) Results The Doppler radar observations were conducted all through the cruise, except over the EEZ without permission. An example of the obtained data are shown in Fig. 3.13-1, for the case when synoptic-scale front passed over the vessel. The meridionally- elongated raining area can be seen in the reflectivity panel. The velocity panel indicates the northerly wind (along front-elongating direction), which can be estimated by strongest approaching (negative) Doppler velocity to the north, and vice versa. Perturbations in the Doppler velocity can be seen to be recognized as wind discontinuous line, wave structure, etc. Detailed analyses of the obtained data will be performed after the cruise. (7) Data archive All data of the Doppler radar observations during this cruise will be submitted to the JAMSTEC Data Management Group (DMG). Table 3.13-1: Operational mode of the radar | Surveil- | | RHI | Vertical | lance | Volume Scan | Scan | Point | PPI Scan | | | Scan ———————————————————————————————————————————————————————————————————————————————— Repeated | 30 | 6 | 12 Cycle (min.) | | | ———————————————————————————————————————————————————————————————————————————————— Times in One | 1 | 1 | 3 | 3 Cycle | | | | ———————————————————————————————————————————————————————————————————————————————— Pulse Width | | | | | | (long/short, | 200/2 | 64/1 | 32/1 | 32/1 | 32/1 | 32/1 in microsec) | | | | | | ———————————————————————————————————————————————————————————————————————————————— Scan Speed | 18 | 18 | 24 | 36 | 9 | 36 (deg/sec) | | | | | | ———————————————————————————————————————————————————————————————————————————————— | | dual PRF (ray alternative) | | | |——————————————————————————————————————| 1250 | 2000 PRF(s) | 400 | 667 | 833 | 938 | 1250 | 1333 | 2000 | | (Hz) | | | | | | | | | ———————————————————————————————————————————————————————————————————————————————— Pulses / Ray | 16 | 26 | 33 | 27 | 34 | 37 | 55 | 32 | 64 ———————————————————————————————————————————————————————————————————————————————— Ray Spacing | 0.7 | 0.7 | 0.7 | 1.0 | 0.2 | 1.0 (deg.) | | | | | | ———————————————————————————————————————————————————————————————————————————————— Azimuth (deg)| Full Circle | Op- | Full | | tion | Circle ———————————————————————————————————————————————————————————————————————————————— Bin Spacing | 150 (m) | ———————————————————————————————————————————————————————————————————————————————— Max. Range | 300 | 150 | 100 | 60 | 100 | 60 (km) | | | | | | ———————————————————————————————————————————————————————————————————————————————— Elevation | 0.5 | 0.5 | 1.0, 1.8, | 18.7, 23.0, | 0.0~ | 90 Angle(s) | | | 2.6, 3.4, | 27.9, 33.5, | 60.0 | (deg.) | | | 4.2, 5.1, | 40.0 | | | | | 6.2, 7.6, | | | | | | 9.7, 12.2, | | | | | | 15.2 | | | Figure 3.13-1: Example of the obtained data, obtained at 2330UTC Jan.02, 2017, when a synoptic-scale front passed over. Upper panel: Radar reflectivity at an elevation of 0.5 degrees, within 300 km radius. Lower panel: Doppler velocity at same elevation angle but within 150 km radius. 3.14 Lidar Observation (1) Personal Masaki KATSUMATA (JAMSTEC) Principal Investigator (onboard Leg-1, not on board Leg-2, 3) Kyoko TANIGUCHI (JAMSTEC) (not on board) Biao GENG (JAMSTEC) (not on board) (2) Objective To capture distributions of cloud, aerosol and water vapor in high temporal and special resolutions. (3) Instrumentation The lidar system on R/V Mirai transmits 10Hz pulse laser at 1064 nm, 532nm, and 355nm, and detects backscattered signals at the same wavelengths (Mie signal) continuously up to 21km height. The system splits signals at 532 nm and 355nm into parallel and perpendicular components. These Mie signals indicate vertical distribution of cloud and aerosol. The parallel and perpendicular components provide the depolarization ratio, an indicator of particle roundness. The combination of these parameters provides the information about the clouds and aerosols, including amounts and types. The system also detects Raman signals at 387nm and 607nm for nitrogen and 660 nm for water vapor. The Raman signals indicate vertical distribution of nitrogen and water vapor molecules. The 660nm and 607nm signals share a 532nm laser as a light source. The ratio of the Raman signals is a proportion to the water vapor mixing ratio, a mass ratio of water vapor and dry air. The observations at 607nm and 660nm are only available at nighttime (from sunset to sunrise). The system reserves a period of 23:56-00:00 UTC for daily maintenance. Instead of observations, the system obtains the background noise data for calibration. Necessary care such as observation window cleaning also take place in the period. (4) Preliminary Results The data were obtained continuously thru Leg-1, 2 and 3, except over the EEZs without permissions. The data will be examined after the cruise. (5) Data Archive All data obtained during this cruise will be submitted to the JAMSTEC Data Management Group (DMG). (6) Acknowledgment During Leg-2 and 3, the operations are supported by the on-board technical staff of Nippon Marine Enterprise Ltd. 3.15 Disdrometers (1) Personnel Masaki KATSUMATA (JAMSTEC) Principal Investigator (on board Leg-1 / not on board Leg-2, 3, 4) Kyoko TANIGUCHI (JAMSTEC) (not on board) Biao GENG (JAMSTEC) (not on board) (2) Objectives The disdrometer can continuously obtain size distribution of raindrops. The objective of this observation is (a) to reveal microphysical characteristics of the rainfall, depends on the type, temporal stage, etc. of the precipitating clouds, (b) to retrieve the coefficient to convert radar reflectivity to the rainfall amount, and (c) to validate the algorithms and the product of the satellite-borne precipitation radars; TRMM/PR and GPM/DPR. (3) Parameters Number and size of precipitating particles (4) Methods Three different types of disdrometers are utilized to obtain better reasonable and accurate value on the moving vessel. Two of them are installed in one place, the starboard side on the roof of the anti- rolling system of R/V Mirai, as in Fig. 3.15-1. The other one, named “micro rain radar”, is installed at the starboard side of the anti- rolling systems (see Fig. 3.15-2). The details of the sensors are described below. All the sensors archive data every one minute. Fig. 3.15-1: The two disdrometers (Parsivel and LPM), installed on the roof of the anti-rolling tank. Fig. 3.15-2: The micro rain radar, installed on the starboard side of the anti-rolling tank. (4-1) Laser Precipitation Monitor (LPM) optical disdrometer The “Laser Precipitation Monitor (LPM)” (Adolf Thies GmbH & Co) is an optical disdrometer. The instrument consists of the transmitter unit which emit the infrared laser, and the receiver unit which detects the intensity of the laser come thru the certain path length in the air. When a precipitating particle fall thru the laser, the received intensity of the laser is reduced. The receiver unit detect the magnitude and the duration of the reduction and then convert them onto particle size and fall speed. The sampling volume, i.e. the size of the laser beam “sheet”, is 20 mm (W) x 228 mm (D) x 0.75 mm (H). The number of particles are categorized by the detected size and fall speed and counted every minutes. The categories are shown in Table 3.15-1. (4-2) “Parsivel” optical disdrometer The “Parsivel” (OTT Hydromet GmbH) is another optical disdrometer. The principle is same as the LPM. The sampling volume, i.e. the size of the laser beam “sheet”, is 30 mm (W) x 180 mm (D). The categories are shown in Table 3.15-2. (4-3) Micro rain radar The MRR-2 (METEK GmbH) was utilized. The specifications are in Table 3.15-3. The antenna unit was installed at the starboard side of the anti- rolling systems (see Fig. 3.15-2), and wired to the junction box and laptop PC inside the vessel. The data was averaged and stored every one minute. The vertical profile of each parameter was obtained every 200 meters in range distance (i.e. height) up to 6200 meters, i.e. well beyond the melting layer. The drop size distribution is recorded, as well as radar reflectivity, path- integrated attenuation, rain rate, liquid water content and fall velocity. (5) Preliminary Results The data were obtained continuously thru the cruise, except over the EEZs without permissions. The result will be examined after the cruise. (6) Data Archive All data obtained during this cruise will be submitted to the JAMSTEC Data Management Group (DMG). (7) Acknowledgment The operations are supported by Japan Aerospace Exploration Agency (JAXA) Precipitation Measurement Mission (PMM). During Leg-2 and 3, the operations are supported by the on-board technical staff of Nippon Marine Enterprise Ltd. Table 3.15-1: Categories of the size and the fall speed for LPM. Particle Size Fall Speed ———————————————————————————— ———————————————————————————— Class Diameter Class width Class Speed Class width [mm] [mm] [m/s] [m/s] ————— ———————— ——————————— ————— ———————— ——————————— 1 ≥ 0.125 0.125 1 ≥ 0.000 0.200 2 ≥ 0.250 0.125 2 ≥ 0.200 0.200 3 ≥ 0.375 0.125 3 ≥ 0.400 0.200 4 ≥ 0.500 0.250 4 ≥ 0.600 0.200 5 ≥ 0.750 0.250 5 ≥ 0.800 0.200 6 ≥ 1.000 0.250 6 ≥ 1.000 0.400 7 ≥ 1.250 0.250 7 ≥ 1.400 0.400 8 ≥ 1.500 0.250 8 ≥ 1.800 0.400 9 ≥ 1.750 0.250 9 ≥ 2.200 0.400 10 ≥ 2.000 0.500 10 ≥ 2.600 0.400 11 ≥ 2.500 0.500 11 ≥ 3.000 0.800 12 ≥ 3.000 0.500 12 ≥ 3.400 0.800 13 ≥ 3.500 0.500 13 ≥ 4.200 0.800 14 ≥ 4.000 0.500 14 ≥ 5.000 0.800 15 ≥ 4.500 0.500 15 ≥ 5.800 0.800 16 ≥ 5.000 0.500 16 ≥ 6.600 0.800 17 ≥ 5.500 0.500 17 ≥ 7.400 0.800 18 ≥ 6.000 0.500 18 ≥ 8.200 0.800 19 ≥ 6.500 0.500 19 ≥ 9.000 1.000 20 ≥ 7.000 0.500 20 ≥ 10.000 10.000 21 ≥ 7.500 0.500 22 ≥ 8.000 unlimited Table 3.15-2: Categories of the size and the fall speed for Parsivel. Particle Size Fall Speed ————————————————————————————— ———————————————————————————— Average Average Class Diameter Class spread Class Speed Class spread [mm] [mm] [m/s] [m/s] ————— ———————— ———————————— ————— ——————— ———————————— 1 0.062 0.125 1 0.050 0.100 2 0.187 0.125 2 0.150 0.100 3 0.312 0.125 3 0.250 0.100 4 0.437 0.125 4 0.350 0.100 5 0.562 0.125 5 0.450 0.100 6 0.687 0.125 6 0.550 0.100 7 0.812 0.125 7 0.650 0.100 8 0.937 0.125 8 0.750 0.100 9 1.062 0.125 9 0.850 0.100 10 1.187 0.125 10 0.950 0.100 11 1.375 0.250 11 1.100 0.200 12 1.625 0.250 12 1.300 0.200 13 1.875 0.250 13 1.500 0.200 14 2.125 0.250 14 1.700 0.200 15 2.375 0.250 15 1.900 0.200 16 2.750 0.500 16 2.200 0.400 17 3.250 0.500 17 2.600 0.400 18 3.750 0.500 18 3.000 0.400 19 4.250 0.500 19 3.400 0.400 20 4.750 0.500 20 3.800 0.400 21 5.500 1.000 21 4.400 0.800 22 6.500 1.000 22 5.200 0.800 23 7.500 1.000 23 6.000 0.800 24 8.500 1.000 24 6.800 0.800 25 9.500 1.000 25 7.600 0.800 26 11.000 2.000 26 8.800 1.600 27 13.000 2.000 27 10.400 1.600 28 15.000 2.000 28 12.000 1.600 29 17.000 2.000 29 13.600 1.600 30 19.000 2.000 30 15.200 1.600 31 21.500 3.000 31 17.600 3.200 32 24.500 3.000 32 20.800 3.200 Table 3.15-3: Specifications of the MRR-2. Transmitter power 50 mW Operating mode FM-CW Frequency 24.230 GHz (modulation 1.5 to 15 MHz) 3dB beam width 1.5 degrees Spurious emission < -80 dBm / MHz Antenna Diameter 600 mm Gain 40.1 dBi 3.16 GNSS precipitable water (1) Personnel Masaki KATSUMATA (JAMSTEC) Principal Investigator (not on board) Mikiko FUJITA (JAMSTEC) (not on board) Kyoko TANIGUCHI (JAMSTEC) (not on board) (2) Objective Recording the GNSS satellite data to estimate the total column integrated water vapor content of the atmosphere. (3) Method The GNSS satellite data was archived to the receiver (Trimble NetR9) with 5 sec interval. The GNSS antenna (Margrin) was set on the roof of radar operation room. The observations were carried out all thru the cruise. (4) Results We will calculate the total column integrated water from observed GNSS satellite data after the cruise. (5) Data archive Raw data is recorded as T02 format and stream data every 5 seconds. These raw datasets are available from Mikiko Fujita of JAMSTEC. Corrected data will be submitted to JAMSTEC Marine-Earth Data and Information Department and will be archived there. 3.17 Ship-borne Measurement of Aerosols (1) Personnel Fumikazu Taketani JAMSTEC PI, not on board Yugo Kanaya JAMSTEC not on board Takuma Miyakawa JAMSTEC on board (Leg 3) Hisahiro Takashima JAMSTEC/Fukuoka Univ. not on board Yutaka Tobo NIPR not on board Yuichi Komazaki JAMSTEC not on board Hitoshi Matsui Nagoya Univ. not on board Momoka Yoshizue Tokyo Univ. of Sci. on board (Leg 3) (2) Objectives • To investigate roles of maritime aerosol particles in climate change through indirect effect (i.e., aerosol-cloud interaction). • To investigate processes of biogeochemical cycles between the atmosphere and sea surface, such as sea spraying process. (3) Parameters • Particle size distributions • Black carbon(BC) and fluorescent aerosol particle number concentrations • Airborne bacteria concentrations • Ice nucleation activity of aerosol particles • Chemical composition of ambient particles • Chemical composition of rain water • Aerosol extinction coefficient (AEC) • Surface carbon monoxide (CO) and ozone(O3) mixing ratios (4) Instruments and methods (4-1) Continuous or temporal aerosol observations: (4-1-1) Particle size distributions The size-resolved number concentration of particles was measured by a scanning mobility particle sizer (SMPS) (comprising a 3080 Electrostatic Classifier with 3081 differential mobility analyzer (DMA), a condensation particle counter (CPC) (model 3010, TSI)), and a handheld optical particle counter (OPC) (KR-12A, RION). We temporally operated the OPC at the time of air sampling on the compass deck (see below for details). (4-1-2) Black carbon (BC) Size-resolved number and mass BC concentrations were measured by an instrument based on laser-induced incandescence, single particle soot photometer (SP2) (model D, Droplet Measurement Technologies). The laser- induced incandescence technique based on intra-cavity Nd:YVO4 laser operating at 1064 nm were used for detection of single particles of BC. (4-1-3) Fluorescence measurements of airborne particles Fluorescent properties of aerosol particles were measured by a single particle fluorescence sensor, Waveband Integrated bioaerosol sensor (WIBS4) (WIBS-4A, Droplet Measurement Technologies). Two pulsed xenon lamps emitting UV light (280 nm and 370 nm) were used for excitation. Fluorescence emitted from a single particle within 310‒400 nm and 420‒650 nm wavelength bands was detected by photomultiplier tubes (PMT) with the bandpass filters. The ambient air was commonly sampled from the rooftop of the environmental research room through a 3-m-long conductive silicone tube to the SP2, SMPS, and WIBS4, and was dehumidified using a Nafion aerosol particle dryer to eliminate liquid water contents of airborne particles (typical relative humidity < 15%). They finally were introduced to those instruments installed in the environmental research room. The OPC instrument was temporally placed on the compass deck at the time to collect the particles for the electron microscopic analyses. (4-2) Aerosol sampling on various types of media Ambient air samplings were carried out using air samplers on the compass deck. Aerosol particles were collected on the quartz fiber (QF) filter (bb= 110 mm) and pre-washed nuclepore membrane filter ((= 47 mm) along cruise track using a high-volume air sampler (HVS, HV-525PM, SIBATA, 500 L/min) and a handmade air sampler (10 L/min) to analyze their composition and ice nuclei ability, respectively. In addition to those samplers, a cascade impactor, which has 5 stages for the size separation, was operated at the flow rate of 9 L/min on the compass deck to investigate the size-resolved chemical compositions. For this sampler, QF filters (FF= 25 mm) were used for the collection. To avoid collecting particles derived from the research vessel exhaust, the sampling period was controlled automatically by using a “wind-direction selection system”. These sampling logs are listed in Tables 3.17-1~3.17-3. Electron microscopic analyses, including Scanning Election Microscopy (SEM) and Transmission Electron Microscopy (TEM), are performed in order to investigate the morphology and physicochemical properties of aerosol particles. For these purposes, aerosol particles were collected on a Silicon wafer or TEM grids (quantifoil or formvar) using air samplers as follows. MPS-3 (California Measurements) for SEM MPS (EcoMesure) for TEM Kl-1L (PIXE INTERNATIONAL) for TEM Sampling was performed on the compass deck for 10 min. These samplings are summarized in Tables 3.17-4. All samples will be analyzed using SEM or TEM placed in a laboratory of JAMSTEC or TUS. Automated counting of autofluorescent and epifluorescent particles were performed using a Bioplorer (Koyo Sangyo). Aerosol particles were collected on the gold-coated membrane filters using a custom-made sampler at typical flow rate of 0.9-1.0 L/min for 2-3 hrs. The collected aerosol particles were analyzed using the Bioplorer immediately after the sampling. The number concentrations of airborne bacteria was calculated by dividing the counted bacteria on a filter by total sampling volume of air. The samples collected were summarized in Table 3.17-5. (4-3) MAX-DOAS Multi-Axis Differential Optical Absorption Spectroscopy (MAX-DOAS), a passive remote sensing technique measuring spectra of scattered visible and ultraviolet (UV) solar radiation, was used for atmospheric aerosol and gas profile measurements. Our MAX-DOAS instrument consists of two main parts: an outdoor telescope unit and an indoor spectrometer (Acton SP-2358 with Princeton Instruments PIXIS-400B), connected to each other by a 14-m bundle optical fiber cable. The line of sight was in the directions of the portside of the vessel and the scanned elevation angles were 1.5, 3, 5, 10, 20, 30, 90 degrees in the 30-min cycle. The roll motion of the ship was measured to autonomously compensate additional motion of the prism, employed for scanning the elevation angle. For the selected spectra recorded with elevation angles with good accuracy, DOAS spectral fitting was performed to quantify the slant column density (SCD) of NO2 (and other gases) and O4 (O2-O2, collision complex of oxygen) for each elevation angle. Then, the O4 SCDs were converted to the aerosol optical depth (AOD) and the vertical profile of aerosol extinction coefficient (AEC) using an optimal estimation inversion method with a radiative transfer model. The tropospheric vertical column/profile of NO2 and other gases were retrieved using derived aerosol profiles. (4-4) CO and O3 Ambient air was continuously sampled on the compass deck and drawn through ~20-m-long Teflon tubes connected to a gas filter correlation CO analyzer (Model 48C, Thermo Fisher Scientific) and a UV photometric ozone analyzer (Model 49C, Thermo Fisher Scientific), located in the Research Information Center. The data will be used for characterizing air mass origins. (4-5) Rain sampling Rain samples were collected using a rain sampler. These samples were analyzed to investigate the chemical composition of rain water over Southern Ocean and south Pacific region. These sampling logs are listed in Tables 3.17-6. (5) Station list or Observation log Air samplings during MR16-09-leg3 were summarized as follows. Table 3.17-1: High-volume air sampling for aerosol composition analyses ID Date and Time Latitude Longitude (deg,min) (deg,min) ——————————— ———————————————————————— ————————— —————————— MR1609-H-S1 2017 02 11 12:40 UTC 60 59 S 77 55 W MR1609-H-S2 2017 02 13 15:07 UTC 64 39 S 98 45 W MR1609-H-S3 2017 02 15 16:31 UTC 66 40 S 121 41 W MR1609-H-S4 2017 02 16 2:50 UTC 67 00 S 126 00 W MR1609-H-S5 2017 02 19 20:15 UTC 60 29 S 126 00 W MR1609-H-S6 2017 02 23 0:00 UTC 53 01 S 126 00 W MR1609-H-S7 2017 02 25 17:40 UTC 51 18 S 143 45 W MR1609-H-S8 2017 02 28 1:00 UTC 46 54 S 158 25 W Table 3.17-2: Low-volume air sampling for the size-resolved aerosol composition analyses ID Date and Time Latitude Longitude (deg,min) (deg,min) —————————— ———————————————————————— ————————— —————————— MR1609-S-1 2017 02 11 12:40 UTC 60 59 S 77 55 W MR1609-S-2 2017 02 15 16:31 UTC 66 41 S 121 40 W MR1609-S-3 2017 02 16 2:50 UTC 67 00 S 126 00 W MR1609-S-4 2017 02 23 0:00 UTC 53 01 S 126 00 W Table 3.17-3: Low-volume air sampling for airborne ice nuclei analysis ID Date and Time Latitude Longitude (deg,min) (deg,min) ———————————— ———————————————————————— ————————— —————————— MR1609-N-001 2017 02 11 12:40 UTC 60 59 S 77 55 W MR1609-N-002 2017 02 13 15:07 UTC 64 39 S 98 45 W MR1609-N-003 2017 02 15 16:31 UTC 66 40 S 125 5 W MR1609-N-004 2017 02 16 2:50 UTC 67 00 S 126 00 W MR1609-N-005 2017 02 18 4:50 UTC 62 59 S 125 59 W MR1609-N-006 2017 02 20 23:55 UTC 57 49 S 126 00 W MR1609-N-007 2017 02 23 0:00 UTC 53 01 S 126 00 W MR1609-N-008 2017 02 24 20:45 UTC 52 14 S 137 17 W MR1609-N-009 2017 02 27 17:12 UTC 47 44 S 156 37 W MR1609-N-010 2017 03 01 2:10 UTC 44 36 S 163 44 W Table 3.17-4: Aerosol sampling for electron microscope analyses ID Date and Time Latitude Longitude (deg,min) (deg,min) —————————————— ———————————————————————— ————————— —————————— MR1609-SEM-01 2017 02 11 12:35 UTC 60 59 S 77 57 W MR1609-SEM-02 2017 02 12 13:02 UTC 63 16 S 87 02 W MR1609-SEM-03 2017 02 13 17:14 UTC 64 45 S 99 46 W MR1609-SEM-04 2017 02 14 15:21 UTC 65 38 S 109 45 W MR1609-SEM-05 2017 02 15 16:27 UTC 66 41 S 121 38 W MR1609-SEM-06 2017 02 16 14:10 UTC 66 21 S 126 03 W MR1609-SEM-07 2017 02 17 12:00 UTC 64 21 S 126 02 W MR1609-SEM-08 2017 02 18 23:15 UTC 62 23 S 126 06 W MR1609-SEM-09 2017 02 19 17:30 UTC 60 29 S 125 59 W MR1609-SEM-10 2017 02 20 14:43 UTC 58 30 S 125 59 W MR1609-SEM-11 2017 02 21 18:45 UTC 55 30 S 125 59 W MR1609-SEM-12 2017 02 22 16:05 UTC 53 30 S 126 01 W MR1609-SEM-13 2017 02 24 16:35 UTC 52 24 S 135 56 W MR1609-SEM-14 2017 02 26 0:09 UTC 50 55 S 145 51 W MR1609-SEM-15 2017 02 26 2:42 UTC 50 45 S 146 41 W MR1609-SEM-16 2017 02 26 19:20 UTC 49 33 S 151 44 W MR1609-SEM-17 2017 02 27 1:12 UTC 49 6.7 S 153 21 W MR1609-SEM-18 2017 02 27 19:07 UTC 47 31 S 157 20 W MR1609-SEM-19 2017 03 02 2:10 UTC 42 20 S 169 20 W MR1609-T-01 2017 02 11 19:45 UTC 61 47 S 80 29 W MR1609-T-02 2017 02 12 20:43 UTC 63 56 S 90 12 W MR1609-T-03 2017 02 13 23:57 UTC 65 2 S 102 52 W MR1609-T-04 2017 02 14 23:52 UTC 65 59 S 113 41 W MR1609-T-05 2017 02 15 0:12 UTC 66 56 S 125 18 W MR1609-T-06 2017 02 16 21:28 UTC 65 40 S 125 58 W MR1609-T-07 2017 02 17 18:20 UTC 63 41 S 126 00 W MR1609-T-08 2017 02 18 23:28 UTC 62 20 S 126 06 W MR1609-T-09 2017 02 19 23:19 UTC 60 01 S 125 58 W MR1609-T-10 2017 02 20 19:45 UTC 58 00 S 126 00 W MR1609-T-11 2017 02 21 18:57 UTC 53 31 S 125 59 W MR1609-T-12 2017 02 25 0:10 UTC 52 05 S 138 25 W MR1609-T-13 2017 02 26 2:30 UTC 50 45 S 146 37 W MR1609-T-14 2017 02 26 17:24 UTC 49 41 S 151 13 W MR1609-T-15 2017 02 27 17:23 UTC 47 42 S 157 01 W MR1609-T-16 2017 03 01 18:35 UTC 43 4 S 167 31 W MR1609-N it-01 2017 02 11 12:37 UTC 61 01 S 77 60 W MR1609-N it-02 2017 02 11 19:45 UTC 61 48 S 81 32 W MR1609-N it-03 2017 02 12 20:43 UTC 63 57 S 90 20 W MR1609-N it-04 2017 02 14 23:57 UTC 65 03 S 102 59 W MR1609-N it-05 2017 02 14 15:21 UTC 65 40 S 109 52 W MR1609-N it-06 2017 02 14 22:52 UTC 65 57 S 113 21 W MR1609-N it-07 2017 02 15 16:21 UTC 66 41 S 121 43 W MR1609-N it-08 2017 02 16 0:11 UTC 66 56 S 125 24 W MR1609-N it-09 2017 02 16 14:10 UTC 66 20 S 126 3 W MR1609-N it-10 2017 02 16 23:25 UTC 65 39 S 125 57 W MR1609-N it-11 2017 02 17 12:15 UTC 64 21 S 126 2 W MR1609-N it-12 2017 02 18 20:40 UTC 62 20 S 126 7 W MR1609-N it-13 2017 02 19 17:33 UTC 60 29 S 125 60 W MR1609-N it-14 2017 02 20 0:01 UTC 60 01 S 125 59 W MR1609-N it-15 2017 02 20 14:50 UTC 58 30 S 125 60 W MR1609-N it-16 2017 02 20 23:41 UTC 57 49 S 125 60 W MR1609-N it-17 2017 02 21 18:45 UTC 55 30 S 125 60 W MR1609-N it-18 2017 02 22 0:10 UTC 55 01 S 125 59 W MR1609-N it-19 2017 02 22 16:10 UTC 53 30 S 126 1 W MR1609-N it-20 2017 02 22 23:40 UTC 53 01 S 126 0 W MR1609-N it-21 2017 02 24 16:35 UTC 52 23 S 136 0 W MR1609-N it-22 2017 02 25 0:10 UTC 52 05 S 138 29 W MR1609-N it-23 2017 02 26 0:09 UTC 50 54 S 145 56 W MR1609-N it-24 2017 02 26 17:24 UTC 49 40 S 151 17 W MR1609-N it-25 2017 02 27 0:54 UTC 49 07 S 153 20 W MR1609-N it-26 2017 02 27 17:24 UTC 47 41 S 157 2 W MR1609-N it-27 2017 02 28 1:58 UTC 46 52 S 158 27 W MR1609-N it-28 2017 02 28 18:23 UTC 45 17 S 161 59 W MR1609-N it-29 2017 03 01 1:57 UTC 44 36 S 163 46 W MR1609-N it-30 2017 03 01 18:35 UTC 43 03 S 167 34 W MR1609-N it-31 2017 03 02 2:10 UTC 42 18 S 169 25 W MR1609-N it-32 2017 03 02 18:30 UTC 40 29 S 173 46 W *MR1609-SEM-## and MR1609-T-## samples were collected by JAMSTEC *MR1609-Nit-## samples were collected by TUS Table 3.17-5: Air sampling for automated counting of airborne bacteria ID Date and Time Latitude Longitude (deg,min) (deg,min) —————————————— ———————————————————————— ————————— —————————— MR1609-B-air01 2017 02 11 12:37 UTC 60 59 S 77 54 W MR1609-B-air02 2017 02 12 13:02 UTC 63 16 S 87 02 W MR1609-B-air03 2017 02 13 17:16 UTC 64 45 S 99 47 W MR1609-B-air04 2017 02 13 20:17 UTC 64 54 S 101 11 W MR1609-B-air05 2017 02 14 15:21 UTC 65 38 S 109 45 W MR1609-B-air06 2017 02 14 18:13 UTC 65 48 S 111 7 W MR1609-B-air07 2017 02 14 20:15 UTC 65 54 S 112 5 W MR1609-B-air08 2017 02 15 16:28 UTC 66 41 S 121 39 W MR1609-B-air09 2017 02 15 19:00 UTC 66 42 S 122 49 W MR1609-B-air10 2017 02 16 2:54 UTC 67 00 S 126 00 W MR1609-B-air11 2017 02 16 14:10 UTC 66 21 S 126 3 W MR1609-B-air12 2017 02 16 21:29 UTC 65 38 S 125 59 W MR1609-B-air13 2017 02 17 12:00 UTC 64 21 S 126 2 W MR1609-B-air14 2017 02 17 18:23 UTC 63 41 S 126 00 W MR1609-B-air15 2017 02 18 1:00 UTC 63 1 S 126 1 W MR1609-B-air16 2017 02 18 18:37 UTC 62 20 S 126 6 W MR1609-B-air17 2017 02 19 17:35 UTC 60 29 S 125 59 W MR1609-B-air18 2017 02 19 23:20 UTC 60 7 S 125 58 W MR1609-B-air19 2017 02 20 14:30 UTC 58 29 S 125 59 W MR1609-B-air20 2017 02 20 19:47 UTC 58 00 S 126 00 W MR1609-B-air21 2017 02 21 18:50 UTC 55 31 S 125 59 W MR1609-B-air22 2017 02 22 16:05 UTC 53 30 S 126 2 W MR1609-B-air23 2017 02 24 16:35 UTC 52 24 S 135 56 W MR1609-B-air24 2017 02 25 0:10 UTC 52 05 S 138 25 W MR1609-B-air25 2017 02 26 0:30 UTC 50 45 S 146 37 W MR1609-B-air26 2017 02 26 17:26 UTC 49 41 S 151 13 W MR1609-B-air27 2017 02 27 0:55 UTC 49 8 S 153 17 W MR1609-B-air28 2017 02 27 17:19 UTC 47 43 S 156 59 W MR1609-B-air29 2017 03 01 2:10 UTC 44 36 S 163 44 W MR1609-B-air30 2017 03 02 2:17 UTC 42 19 S 169 22 W Table 3.17-6: Rain sampling for chemical composition analysis ID Date and Time Latitude Longitude (deg,min) (deg,min) ————————————————————————— ———————————————————————— ————————— —————————— MR 1609-Leg3-rain-001-冷凍 2017 02 11 12:45 UTC 61 01 S 77 60 W MR 1609-Leg3-rain-001-冷蔵 2017 02 11 12:45 UTC 61 01 S 77 60 W MR 1609-Leg3-rain-002-冷凍 2017 02 12 20:45 UTC 63 57 S 90 20 W MR 1609-Leg3-rain-003-冷凍 2017 02 15 16:30 UTC 66 41 S 121 43 W MR 1609-Leg3-rain-003-冷蔵 2017 02 15 16:30 UTC 66 41 S 121 43 W MR 1609-Leg3-rain-004-冷凍 2017 02 16 23:30 UTC 65 39 S 125 57 W MR 1609-Leg3-rain-005-冷凍 2017 02 18 0:27 UTC 63 06 S 126 1 W MR 1609-Leg3-rain-006-冷凍 2017 02 18 23:25 UTC 62 20 S 126 7 W MR 1609-Leg3-rain-007-冷凍 2017 02 20 23:59 UTC 57 48 S 125 60 W MR 1609-Leg3-rain-008-冷凍 2017 02 22 0:27 UTC 55 01 S 125 59 W MR 1609-Leg3-rain-009-冷凍 2017 02 23 0:03 UTC 53 02 S 126 0 W MR 1609-Leg3-rain-009-冷蔵 2017 02 23 0:03 UTC 53 02 S 126 0 W MR 1609-Leg3-rain-010-冷凍 2017 02 24 16:54 UTC 52 23 S 136 1 W MR 1609-Leg3-rain-010-冷蔵 2017 02 24 16:54 UTC 52 23 S 136 1 W MR 1609-Leg3-rain-011-冷凍 2017 02 25 0:29 UTC 52 05 S 138 30 W MR 1609-Leg3-rain-012-冷凍 2017 02 27 17:44 UTC 47 40 S 157 4 W MR 1609-Leg3-rain-012-冷蔵 2017 02 27 17:44 UTC 47 40 S 157 4 W MR 1609-Leg3-rain-013-冷凍 2017 02 28 18:38 UTC 45 18 S 161 58 W MR 1609-Leg3-rain-013-冷蔵 2017 02 28 18:38 UTC 45 18 S 161 58 W MR 1609-Leg3-rain-014-冷凍 2017 03 02 18:43 UTC 40 29 S 173 45 W MR 1609-Leg3-rain-014-冷蔵 2017 03 02 18:43 UTC 40 29 S 173 45 W (6) Preliminary results Figure 3.17-1: Average particle size distribution for Feb 11 – 28, 2017. (X axis is Particle diameter in nm; Y axis is the number concentration normalized by size-bin width) Figure 3.17-2: Histogram of total particle number concentration for Feb 11-28, 2017. (7) Data archives These data obtained in this cruise will be submitted to the Data Management Group of JAMSTEC, and will be opened to the public via “Data Research System for Whole Cruise Information in JAMSTEC (DARWIN)” in JAMSTEC web site. 3.18 Underway CT (1) Personnel Akihiko Murata (JAMSTEC) Tomonori Watai (MWJ) Atsushi Ono (MWJ) Emi Deguchi (MWJ) Nagisa Fujiki (MWJ) (2) Objective It is doubtless that the ocean moderates global warming by absorbing ~30% of anthropogenic CO2 emitted into the atmosphere. However, increases of anthropogenic CO2 in the ocean cause another CO2 problem called as ocean acidification. Since it is predicted that ocean acidification gives a large influence on ocean biology, especially on calcifying organisms, it is an important task to evaluate progression of ocean acidification. In the leg 3 of MR16-09 cruise, we measured underway dissolved inorganic carbon (CT) in the surface seawater continuously along the cruise track. The data for CT are used to calculate saturation state of calcium carbonate (a), which is one of good indicators of ocean acidification, together with data for underway pCO2 (section 3.7) (3) Apparatus Measurement of CT was made with automated TCO2 analyzer (Nippon ANS, Inc., Japan). The system comprises of a seawater dispensing system, a CO2 extraction system and a coulometer (Model 3000A, Nippon ANS, Inc., Japan). Specification of the system is as follows: Seawater collected from the seawater inlet at 4.5 m deep is transferred into a DURAN® glass bottle of nominal 250 ml after overflowing seawater of 3 time volume of the bottle. The seawater sample is kept at 20°C by a constant temperature bath until measurement. Then the seawater sample is dispensed from the glass bottle into a pipette of about 15 ml volume. The pipette is also kept at 20 °C by a water jacket, in which water from a water bath set at 20°C is circulated. CO2 dissolved in a seawater sample is extracted in a stripping chamber of the CO2 extraction system by adding phosphoric acid (~ 10 % v/v) of about 2 ml. The stripping chamber is approx. 25 cm long and has a fine frit at the bottom. The acid is added to the stripping chamber from the bottom of the chamber by pressurizing an acid bottle for a given time to push out the right amount of acid. The pressurizing is made with nitrogen gas (99.9999 %). After the acid is transferred to the stripping chamber, a seawater sample kept in a pipette is introduced to the stripping chamber by the same method as in adding an acid. The seawater reacted with phosphoric acid is stripped of CO2 by bubbling the nitrogen gas through a fine frit at the bottom of the stripping chamber. The CO2 stripped in the chamber is carried by the nitrogen gas (flow rates is 140 ml min-1) to the coulometer through a dehydrating module. The module consists of two electric dehumidifiers (kept at ~4°C) and a chemical desiccant (Mg(ClO4)2). The measurement sequence such as 1.5% CO2 gas in N2 base, system blank (phosphoric acid blank), seawater samples (6) is repeated automatically by PC control. (4) Results Concentrations of CT in surface seawater along the cruise track are shown in Fig. 3.18.1, together with (a) salinity and (b) SST. Fig. 3.18.1: Preliminary results of concentrations of CT in surface seawater (blue), salinity (red), and SST (green) observed during the leg 3 of MR16-09. 3.19 XCTD March 3, 2017 (1) Personnel Hiroshi Uchida (JAMSTEC) Shinya Okumura (NME) Koichi Inagaki (NME) Ryo Kimura (NME) Masanori Murakami (Mirai crew) (2) Objectives XCTD (eXpendable Conductivity, Temperature and Depth profiler) measurements were carried out to substitute CTD casts and to evaluate the fall rate equation and the thermal bias by comparing with CTD (Conductivity, Temperature and Depth profiler) measurements. (3) Instrument and Method The XCTD used was XCTD-4 (Tsurumi-Seiki Co., Ltd., Yokohama, Kanagawa, Japan) with an MK-150N deck unit (Tsurumi-Seiki Co., Ltd.). The manufacturer’s specifications are listed in Table 3.19.1. In this cruise, the XCTD probes were deployed by using 8-loading automatic launcher (Tsurumi-Seiki Co., Ltd.) or a hand launcher (stn. ****). For comparison with CTD, XCTD was deployed at about 10 minutes after the beginning of the down cast of the CTD (P17E_8, 16, 22 and 23). For correction of the sound velocity profile used in the bathymetry observation, XCTD-1 was deployed near station P17E_1. Also, two XCTD-4 were deployed at CO2 buoy deployment locations at longitude of 140°W and 160°W. The fall-rate equation provided by the manufacturer was initially used to infer depth Z (m), Z = at – bt2, where t is the elapsed time in seconds from probe entry into the water, and a (terminal velocity) and b (acceleration) are the empirical coefficients (Table 3.19.2). (4) Data Processing and Quality Control The XCTD data were processed and quality controlled based on a method by Uchida et al. (2011). Differences between XCTD and CTD depths were shown in Fig. 3.19.1. The terminal velocity error was estimated for the XCTD-4 (Table 3.19.2). The XCTD-4 data were corrected for the depth error by using the estimated terminal velocities. Differences of temperature on pressure surfaces were examined by using side-by-side XCTD and CTD data (Fig. 3.19.3). Average thermal bias below 900 dbar was 0.014 °C. The XCTD data were corrected for the thermal bias. Differences of salinity on reference temperature surfaces were examined by using CTD data (Fig. 3.19.4). The XCTD data were corrected for the estimated salinity bias. (5) Results Temperature-salinity plot using the quality controlled XCTD data is shown in Fig. 3.19.3. (6) References Kizu, S., H. Onishi, T. Suga, K. Hanawa, T. Watanabe, and H. Iwamiya (2008): Evaluation of the fall rates of the present and developmental XCTDs. Deep-Sea Res I, 55, 571–586. Uchida, H., K. Shimada, and T. Kawano (2011): A method for data processing to obtain high-quality XCTD data. J. Atmos. Oceanic Technol., 28, 816–826. Uchida, H., A. Murata, and T. Doi (eds.) (2014): WHP P10 Revisit in 2011 Data Book, 179 pp., JAMSTEC. Uchida, H., K. Katsumata, and T. Doi (eds.) (2015): WHP P14S/S04I Revisit in 2012/2013 Data Book, 187 pp., JAMSTEC. Uchida, H and T. Doi (eds.) (2016): WHP P01 Revisit in 2014 Data Book, 149 pp., JAMSTEC, ISBN 978-4-901833-22-6. Table 3.19.1: Manufacturer’s specifications of XCTD-4. Parameter Range Accuracy ———————————— ——————————————— ————————————————————————————————— Conductivity 0 ~ 60 mS cm–1 ±0.03 mS cm–1 Temperature –2 ~ 35 °C ±0.02 °C Depth 0 ~ 1850 m 5 m or 2%, whichever is greater * ———————————————————————————————————————————————————————————————— * Depth error is shown in Kizu et al (2008). Table 3.19.2: Manufacturer’s coefficients for the fall-rate equation. Model a b e (terminal velocity, m/s) (acceleration, m/s2) (terminal velocity error, m/s) —————— ———————————————————————— ———————————————————— —————————————————— XCTD-4 3.68081 0.00047 –0.0197 Table 3.19.3: Thermal biases of the XCTD temperature data. Cruise Average thermal bias (°C) Depth range Source ——————— ————————————————————————— ———————————— ———————————————————————— MR09-01 0.016 >= 1100 dbar Uchida et al. (2011) KH-02-3 0.019 >= 1100 dbar Uchida et al. (2011) MR11-08 0.014 >= 1100 dbar Uchida et al. (2014) MR12-05 0.009 >= 400 dbar Uchida et al. (2015) MR14-04 0.011 >= 900 dbar Uchida et al. (2016) MR15-05 –0.003 >= 900 dbar Cruise report of MR15-05 MR16-09 0.014 >= 900 dbar this report Mean 0.011 ± 0.007 Table 3.19.4: Salinity biases of the XCTD data. XCTD Salinity Reference Reference Reference station bias temperature (°C) salinity CTD stations ——————— ———————— ———————————————— ————————— ———————————— 8 –0.007 1.7 34.7306 7, 8, 9 22 0.008 2.4 34.6366 22, 23 23 0.017 2.4 34.6366 22, 23 Figure 3.19.1: Differences between XCTD and CTD depths for XCTD-4. Differences were estimated with the same method as Uchida et al. (2011). Standard deviation of the estimates (horizontal bars) and the manufacturer’s specification for XCTD depth error (dotted lines) are shown. The regression for the data (solid line) is also shown. Figure 3.19.2: Comparison between XCTD and CTD temperature profiles. (a) Mean temperature of CTD profiles with standard deviation (shade) and (b) mean temperature difference with standard deviation (shade) between the XCTD and CTD. Mean profiles were low-pass filtered by a running mean with a window of 51 dbar. Figure 3.19.3: Comparison of temperature-salinity profiles of CTD data (red lines) used for the XCTD salinity bias estimation and salinity bias-corrected XCTD data (black lines). 3.20 Radiosonde observations (1) Personnel Masaki KATSUMATA (JAMSTEC) Principal Investigator (on board Leg-1) Biao GENG (JAMSTEC) (not on board) Kyoko TANIGUCHI (JAMSTEC) (not on board) Soichiro SUEYOSHI (NME) Operation Leader Yutaro MURAKAMI (NME) (2) Objectives The objective of radiosonde observations is to obtain the atmospheric profile of temperature, humidity, and wind speed/direction, and their temporal and special variations over the tropical ocean. (3) Operational methodology The Vaisala GPS radiosonde sensors (RS92-SGPD and RS41-SGP) were launched with the balloon (TA-200). The on-board radiosonde system consists of sounding processing system (SPS-311), ground check device (RI41), processing and recording software (MW41), GPS antenna (GA20), UHF antenna (RB21), and automatic balloon launcher (ASAP). In addition, the pressure sensor (PTB-330) was also utilized for ground check. In case the relative wind to the ship is not appropriate for using the automatic balloon launcher, the radiosonde equipped balloon was launched manually. (4) Results The radiosonde observations were conducted from Dec. 29, 2016 to Jan.15, 2017. During this period, 51 radiosondes equipped balloons have been launched (Table 3.20-1). Figure 3.20-1 shows some results of the radiosonde observations. Detailed analyses of the data observed by the radiosonde will be performed after the cruise. (5) Data Archive The radiosonde data were sent to the world meteorological community via Global Telecommunication System (GTS) through the Japan Meteorological Agency, immediately after each observation, when the appropriate satellite communication was available. Raw data are recorded in Vaisala original binary format. The ASCII data are also available. These datasets will be submitted to JAMSTEC Data Integration and Analyses Group. Table 3.20-1: Radiosonde launch log, with surface values and maximum height. Nominal Time Launched Location Surface Values Max ID YYYYMMDD Lat. Lon. P T RH WD WS Height Sensor hh deg.N deg.E hPa deg.C % Deg. m/s m Type ————— ———————————— ——————— ———————— —————— ————— —— ——— ———— ————— ——————— RS001 2016122900 -26.051 -174.346 1006.3 22.6 80 147 9.4 22045 RS002 2016122912 -27.451 -172.664 1004.5 22.0 87 141 7.9 22486 RS003 2016123000 -29.027 -170.693 1003.7 21.2 93 174 4.5 22898 RS004 2016123012 -30.633 -168.564 1005.0 21.9 92 51 4.5 22986 RS005 2016123100 -32.268 -166.310 1008.5 21.6 90 51 5.9 18582 RS006 2016123112 -33.824 -163.983 1012.4 20.7 91 90 3.2 29246 RS007 2017010100 -35.343 -161.605 1016.0 20.3 91 58 8.5 20797 RS008 2017010106 -36.071 -160.380 1017.1 20.2 86 48 7.1 21961 RS009 2017010112 -36.807 -159.130 1016.8 19.3 84 61 6.9 20864 RS010 2017010118 -37.504 -157.821 1016.8 18.8 87 58 8.0 22280 RS011 2017010200 -38.186 -156.538 1015.1 19.2 81 32 6.9 20785 RS012 2017010206 -38.882 -155.204 1012.6 18.4 90 26 7.2 20394 RS013 2017010212 -37.576 -153.732 1009.1 17.6 94 14 8.5 21372 RS92 RS014 2017010218 -40.250 -152.311 1005.8 16.9 96 11 9.3 19666 RS015 2017010300 -40.934 -150.872 1002.4 15.4 90 358 12.2 24105 RS016 2017010306 -41.537 -149.377 999.8 16.0 98 353 13.8 18075 RS017 2017010312 -42.115 -147.839 999.4 15.4 100 345 10.4 16678 RS018 2017010318 -42.733 -146.302 1002.4 12.5 100 186 11.4 18540 RS019 2017010400 -43.190 -145.013 1004.1 12.3 100 165 8.6 21521 RS020 2017010412 -44.149 -142.101 1007.4 11.5 96 171 7.7 20735 RS021 2017010500 -44.931 -139.159 1011.3 13.0 99 336 5.6 22752 RS022 2017010512 -45.947 -135.890 1015.1 12.9 99 328 5.6 21786 RS023 2017010600 -46.748 -132.380 1017.8 12.8 96 326 5.8 22231 RS024 2017010612 -47.433 -128.840 1018.3 12.2 97 336 5.3 21201 RS025 2017010700 -48.042 -125.109 1020.0 12.3 93 348 3.5 21294 RS026 2017010709 -48.367 -122.338 1022.4 11.7 78 32 2.7 20378 RS027 2017010712 -48.474 -121.398 1022.5 11.0 88 71 2.5 20800 RS028 2017010800 -48.773 -118.048 1025.3 10.9 86 241 1.7 18227 RS029 2017010809 -48.964 -115.406 1026.5 9.5 73 173 5.8 23324 RS030 2017010812 -49.024 -114.639 1025.9 8.9 73 200 6.0 19343 RS031 2017010900 -49.080 -111.410 1025.0 8.5 77 217 3.2 21872 RS032 2017010906 -49.097 -109.733 1024.6 8.4 79 206 4.2 21216 RS033 2017010912 -49.100 -108.011 1022.3 8.8 84 216 5.1 22195 RS034 2017011000 -49.045 -105.042 1019.1 8.1 87 207 3.2 19971 RS035 2017011006 -48.969 -103.614 1019.0 8.7 97 149 4.0 18118 RS036 2017011012 -48.875 -102.260 1017.8 8.2 83 168 3.4 21405 RS037 2017011100 -48.703 -99.463 1016.2 9.1 76 214 1.2 20638 RS038 2017011106 -48.542 -98.030 1015.8 9.0 71 227 2.7 21070 RS41 RS039 2017011112 -48.408 -96.661 1014.1 7.6 91 245 5.5 20946 RS040 2017011200 -48.055 -93.844 1012.5 10.2 79 254 11.2 20429 RS041 2017011206 -47.846 -92.544 1013.5 9.3 84 218 9.8 21518 RS042 2017011212 -47.680 -91.152 1014.6 9.9 86 240 10.3 17657 RS043 2017011300 -47.219 -88.682 1018.3 10.5 81 264 8.9 20881 RS044 2017011306 -46.952 -87.362 1019.5 10.4 82 263 11.2 21297 RS045 2017011312 -46.697 -86.093 1019.5 10.8 75 264 10.7 21013 RS046 2017011400 -45.920 -82.622 1018.5 11.8 75 264 11.2 22353 RS047 2017011406 -45.496 -81.002 1017.4 11.8 65 259 11.1 19633 RS048 2017011412 -44.940 -80.049 1016.3 11.7 69 276 8.6 20843 RS049 2017011418 -44.661 -80.139 1015.3 10.9 86 269 9.1 21309 RS050 2917011500 -44.542 -80.109 1013.7 11.6 93 295 5.3 21899 RS051 2017011506 -44.396 -80.021 1011.5 12.6 85 321 9.8 21741 Figure 3.20-1: Time-height (time-pressure) cross section of the obtained data, for (top) potential temperature, (second top) relative humidity, (third) zonal wind, and (bottom) meridional wind, respectively. 4. Station Observation 4.1 Single Channel Seismic Survey (1) Personnel Natsue Abe (R&D Center for Ocean Drilling Science, JAMSTEC) Toshimasa Nasu (Nippon Marine Einterprises,Ink.) Mitsuteru Kuno (Nippon Marine Einterprises,Ink.) Satsuki Iijima (Nippon Marine Einterprises,Ink.) Hiroyuki Hayashi (Nippon Marine Einterprises,Ink.) (2) Introduction The SCS reflection data were acquired along 4 lines (L1 ~4), listed below, in two areas with a total length of approximately 240 km (Figures 4.1.1&2; Table 4-1-1). ・Line1:Start 45-56.33835S, 75-56.36719W - End 46-06.71562S, 76-43.73703W ・Line2:Start 45-55.04196S, 75-50.95871W - End 45-58.12477S, 76-04.74792W ・Line3:Start 47-52.64648S, 75-56.24817W – End 47-52.52037S, 76-50.38330W ・Line4_0: Start 47-57.88422S, 75-57.24289W – End 47-57.29004S, 76-01.83151W ・Line4_1: Start 47-57.23190S, 76-02.19543W - End47-51.93878S, 76-46.98715W In all tracks, reflection from the seafloor was clearly recorded. Igneous basement structures were confirmed except beneath steep slope of the ridge-like seamounts and the continental slops. In some places beneath the continental slops, the boundary between the footwall and the hanging wall is likely identified (Lines 3 & 4). In the L1&2, half graben structure that was formed during mid-ocean ridge opening are clear reflections were recognized within both sediments and basements. The SCS reflection data across the subduction zone are complex. Further descriptions and investigations will be reported later. (3) Spec information The single channel seismic survey equipment and specification is as follows. The image of the single channel seismic system if shown in the Figure 4.1.3. The detail conditions of each lines are listed in the Table 4.1.2. Streamer Manufacturer: S.I.G Active section length: 65 m Hydrophone Interval: 1 m Type of Hydrophone: S.I.G.16 Hydrophone output: -90 dB,re 1V/µbar, ±1 dB Frequency flat from: 10Hz to 1000Hz Depth sensor: Yes Preamplifier gain: 39 Lead in cable length: 135 m Receiver depth: 9.62 m (Line1), 1.91 m (Line2), 1.75 m (Line3), 1.85 m (Line4_0), 2.19 m (Line4_0) Source Manufacturer: Sercel Type of airgun: GI Gun Volume: 150 cu.in (G:45 cu.in, I:105 cu.in) Air pressure: 13.5MPa Source depth: 2 m Depth sensor: No Gun Controller: Hotshot ver. 3.3000 Air Compressor Manufacturer: Service Engineering co., ltd Type of machine: 4SA30-A150K Air supply Capacity: 2.0 m3/min. Recording System Manufacturer: GEOMETRICS Type of system: Geode ver. 11.1.69.0 Recording format: SEG-D 8058 Rev.1 Recording length: 7,500 msec Water Delay: 0 msec Sample rate: 1 msec High cut filter: None Low cut filter: None Recording media: Hard Disk GPS System Manufacturer: Fugro Type of system: MultiFix6 DGPS Reference Station: G2 Reference Station (ASAT) Navigation System Manufacturer: MARIMEX JAPAN Type of system: Nav log ver. 2.2.7 Shot Point Geometry Time mode shooting: ture mode Geodetic Parameter Spheroid: WGS84 Semi-major Axis: 6,378,137 m Inverse Flattening: 298.26 Projection: U.T.M Zone18 (4) Data process and Archives Figure 4-1-4 shows the data processing flow to filtered section. Other details of data acquisition and processing of Single channel seismic survey are attached as below. Data Nav_Raw (.csv format): position logging data SEG-D_Raw (.sgd format): Raw data SEG-Y_Raw (.sgy): Transform data into SEG-Y from SEG-D_Raw data SEG-Y_filetr (.seg): Filtering data of SEG-Y BMP (.BMP format) Bitmap profile of SEG-Y data for each lines. Fig.4-1-2: The location of SCS survey lines 3 and 4. Table 4-1-1: Position, length and the azimuth in formation of each survey line. NME SINGLE CHANNEL SEISMIC SURVEY LINE LIST MR16-09_leg.2 Direc- Line Date Time Passing Shot Vessel Position Length tion No. (UTC) (UTC) Point No. Lat. Lon. [m] [deg] ———— ————————— ———————— ——————— ———— ———————————— ———————————— ———————— —————— 1 2017/1/23 2:24:43 F.S.P 1001 45-56.33835S 75-56.36719W 64,063.3 251.51 2017/1/23 3:05:43 F.G.S.P 1174 45-57.06688S 75-59.90295W 2017/1/23 10:54:06 L.G.S.P 3682 46-06.62773S 76-43.32138W 2017/1/23 10:58:50 L.S.P 3705 46-06.71562S 76-43.73703W 2 2017/1/25 2:17:12 F.S.P 1001 45-55.04196S 75-50.95871W 18,707.9 251.51 2017/1/25 2:17:12 F.G.S.P 1001 45-55.04196S 75-50.95871W 2017/1/25 4:57:26 L.G.S.P 1794 45-58.12477S 76-04.74792W 2017/1/25 4:57:26 L.S.P 1794 45-58.12477S 76-04.74792W 3_0* 2017/1/26 20:23:00 F.S.P 1001 47-52.64648S 75-56.24817W 67,473.6 269.01 2017/1/26 20:23:00 F.G.S.P 1001 47-52.64648S 75-56.24817W 2017/1/27 5:58:29 L.G.S.P 3859 47-52.52037S 76-50.38330W 2017/1/27 5:58:29 L.S.P 3859 47-52.52037S 76-50.38330W 4_0 2017/1/28 21:24:31 F.S.P 1001 47-57.88422S 75-57.24289W 4,983.2 278.96 2017/1/28 21:24:31 F.G.S.P 1001 47-56.75629S 75-57.24289W 2017/1/29 22:15:20 L.G.S.P 1253 47-57.37907S 76-01.17737W 2017/1/29 22:15:20 L.G.S.P 1253 47-57.37907S 76-01.17737W 4_1† 2017/1/28 22:34:36 F.S.P 1001 47-57.23190S 76-02.19543W 56,647.4 278.96 2017/1/28 22:34:36 F.G.S.P 1001 47-57.23190S 76-02.19543W 2017/1/29 7:59:55 L.G.S.P 3807 47-51.93878S 76-46.98715W 2017/1/29 7:59:55 L.S.P 3807 47-51.93878S 76-46.98715W ————————————————————————————————————————————————————————————————————————————————————————— *SP No.2737 - SP No.2788 = Point 76-28W transit. SP3456(FF3456) is most close to Line4_1. †SP3514(FF3514) is most close to Line3. Fig. 4-1-3: Image of the Single Channel Seismic Survey system. Fig. 4-1-4: Seismic data processing flow to filtered section for MR16-09 Leg 2. 4.2 Sediment Core 4.2.1 Site survey (bathymetry and sediment structure) observations (1) Personnel Kana Nagashima (JAMSTEC); nagashimak@jamstec.go.jp Frank Lamy (Alfred Wegener Institute); Frank.Lamy@awi.de Helge Arz (Ernst-Moritz-Arndt-University Greifswald); helge.arz@io-warnemuende.de Wataru Tokunaga (NME), Operation Leader; tokunagaw@nme.co.jp Koichi Inagaki (NME); inagakik@nme.co.jp Yutaro Murakami (NME); murakamiy@nme.co.jp (2) Objective To find best location taking the sediment for paleoceanography, site survey was conducted using the Multi-narrow Beam Echo Sounding system (MBES), SEABEAM 3012 (L3 Communications ELAC Nautik GmbH) and Sub-Bottom Profiler (SBP), Bathy 2010 (SyQwest Incorporated) on R/V MIRAI. SBP system collected vertical information of sediments. (3) Measured parameters System configuration, performance and data acquisition of SEABEAM 3012 and Bathy 2010 systems showed “3.2 Bathymetry (Sea beam, sub-bottom profiler)”. (4) Preliminary results Figures 4.2.1-1 to 4.2.1-5 show survey maps and sub-bottom profiles for Station 02, 03, 08 and 10. Sediment coring was conducted at the stations using multiple piston coring system. Geographic positions of each station were shown in Table 4.2.1-1 below. (5)Date archive All data are submitted to JAMSTEC Data Management Group (DMG) and is currently under its control and will be opened to public via “R/V MIRAI Data Web Page” in JAMSTEC homepage. Table 4.2.1-1: Position of each coring station during MR16-09 Leg.2 cruise Date Sta- Water Position Core (UTC) Core tion Depth Latitude Longitude Length yyyymmdd ID Name Location (m) (°S) (°W) (cm) ————————— ———— ————— —————————— ————— —————————— —————————— —————— 2017/1/22 PC01 St.02 Guafo Area 1,535 46-04.2714 75-41.2293 534.5 2017/1/22 MC01 St.02 Guafo Area 1,537 46-04.2885 75-41.2226 - 2017/1/23 PC02 St.03 Off Taitao 2,793 46-04.2316 76-32.0952 1273.0 2017/1/23 MC02 St.03 Off Taitao 2,787 46-04.2249 76-32.0902 - 2017/1/27 PC03 St.08 Off Taitao 3,082 46-24.3180 77-19.4499 1753.0 2017/1/31 PC04 St.10 Off Chile 3,848 50-48.3254 79-07.0752 1695.0 2017/1/31 MC04 St.10 Off Chile 3,851 50-48.3381 79-07.0823 - Fig. 4.2.1-1: Bathymetric map (left) and sub-bottom profile (right) around station 02 (coring site of PC01 and MC01). Fig. 4.2.1-2: Bathymetric map (top) and sub-bottom profile (bottom) around station 03 (coring site of PC02 and MC02). Fig. 4.2.1-3: Bathymetric map (top) and sub-bottom profile (bottom) around station 08 (coring site of PC03). Fig. 4.2.1-4: Bathymetric map (left) and sub-bottom profile (right) around station 10 (coring site of PC04 and MC04). 4.2.2 Piston corer system (PC) (1) Personnel Yusuke Sato (Marine Works Japan Co. Ltd); satoy@mwj.co.jp Ei Hatakeyama (Marine Works Japan Co. Ltd); hatakeyamae@mwj.co.jp Yohei Katayama (Marine Works Japan Co. Ltd); katayamay@mwj.co.jp (2) Objective Collection of sea floor sediment (3) Instruments and Method The piston corer system (PC) is composed of the head of the corer, barrels, piston, catcher, bit, trigger and pilot core sampler. The duralumin pipes are used for the barrel. A total of 15 or 20 m-long duralumin pipe is composed of three or four 5 m segments which are combined one another by stainless joint sleeves. We used a 74 mm long type pilot corer for a pilot core sampler. We used inner liners: polycarbonate liner tubes (Inner type). A compass with inclinometer was attached above the weight of the corer to examine performance of the PC. Diagram of PC is shown in the Fig. 4.2.2-1. In the Inner type piston corer, it pulls out inner tubes only from the duralumin pipes and the sediment can be collected. The inner tubes filled by sediments are cut with the handy cutter every 1 m after taking out from the barrel. The sediment sections are longitudinally cut into working and archive halves by a splitting devise and a stainless wire. After splitting, both cores are putted white pins at interval of 2 cm and orange pins at interval of 10 cm. Specification of the piston corer system is shown below. Head of the corer Main unit (Stainless, Lead): Weight; 1.3 ton Barrel (Duralumin): Length; 5 m Inner diameter; 80 mm Outer diameter; 92 mm Inner tube (Polycarbonate): Length; 5 m Inner diameter; 74 mm Outer diameter; 78 mm (4) Winch operation When we started lowering, a speed of wire out was set to be 0.2 m/s., and then gradually increased to the maximum of 1.0 m/s. PC were stopped at a depth about 100 m above the sea floor for 3 minutes to reduce any pendulum motion of the system. After the PC were stabilized, the wire was stored out at a speed of 0.3 m/s, and we carefully watched a tension meter. When the corers touched the bottom, wire tension abruptly decreases by the loss of the corer weight. Immediately after confirmation that the PC hit the bottom, wire out was stopped and rewinding of the wire was started at a dead slow speed (~0.3 m/s.), until the tension gauge indicates that the PC were lifted off the bottom. After leaving the bottom, winch wire was wound in at the maximum speed. (5) Results Details of coring positions and core lengths are shown are shown in Table 4.2.1-1 and Appendix 1 (Coring information). Fig. 4.2.2-1: Diagram of Piston corer system. 4.2.3 Multiple Corer system (MC) (1) Personnel Yusuke Sato (Marine Works Japan Co. Ltd); satoy@mwj.co.jp Ei Hatakeyama (Marine Works Japan Co. Ltd); hatakeyamae@mwj.co.jp Yohei Katayama (Marine Works Japan Co. Ltd); katayamay@mwj.co.jp (2) Objective Collection of surface sediment (3) Instruments and Methods Multiple corer (MC) consists of body (620 kg in weight) and eight sub-corer attachments. Acryl pipe and polycarbonate pipe are used for the sediment coring. The pipes are 60 cm in length, and the diameter is 74 mm. For MC02 and MC04, attached Water sampling system without off line camera and light. Water sampling system attaches four Niskin bottles (8- liter), SBE 39 temperature (pressure optional) recorder and Magnet switch data logger to the body. (4) Winch Operation When we starts lowering the MC, a speed of wire out is set to be 0.2 m/s., and then gradually increased to be 1.0 m/s. The MC is stopped at a depth about 50 m above the sea floor for 3 minutes to reduce any pendulum motion of the sampler. After the sampler is stabilized, the wire is stored out at a speed of 0.3 m/s., and we carefully watch a tension meter. When the MC touches the bottom, wire tension leniently decreases by the loss of the sampler weight. After confirmation that the MC touch seafloor, the wire out is stopped then another 3~5 m rewinding. The wire is started at dead slow speed, until the tension gauge indicates that the corer is lifted off the bottom. After leaving the bottom, which wire is wound in at the maximum speed. The MC came back ship deck, sub-corer attachments and Niskin bottles or off line camera were detached from the main body. (5) Results Details of coring position and core length are shown in the Appendix 1 (Coring Information) 4.2.4 Multi sensor core logger (MSCL) (1) Personnel: Kazuma Takahashi (Marine Works Japan Ltd.); takahashik@mwj.co.jp (2) Objectives To understand characteristics of sediment samples and to correlate different cores, physical properties, magnetic susceptibility was taken by using the whole round core sections before splitting and the GEOTEC multi-sensor core logger (MSCL). (3) Measured Parameters MSCL has sensors of the gamma-ray attenuation (GRA), the P-wave velocity (PWV) and the magnetic susceptibility (MS). Whole-core samples are used for the logger measurements. (4) Instruments and Methods Whole-core samples are kept in the laboratory for the night to equalize the sediment temperature with the room temperature. Measurement interval was every 1 cm for all cores (Only PC01 core was measured by 2 cm interval). GRA is measured a gamma ray source and a detector, which are mounted on the center sensor stand. A narrow beam of gamma ray is emitted by Cesium-137 (137Cs, energies principally at 0.662 MeV). The detector comprises a scintillator (a 2” diameter and 2” thick NaI crystal). The photon of gamma ray is collimated through 5 mm diameter in rotating shutter at the front of the housing of 137Cs. These photons pass through the center of the whole core and are detected the scintillation detector on the other side. The detector comprises a scintillator (a 2” diameter and 2” thick NaI crystal). The calibration of GRA assumes a two-phase system model for sediments, where the two phases are the minerals and the interstitial water. Aluminum has an attenuation coefficient similar to common minerals and is used as the mineral phase standard. Pure water is substituted as the interstitial-water phase standard. The actual standard consists of a telescoping aluminum rob (five elements of varying thickness) mounted in a piece of core liner and filled with pure water. GRA was measured with 10 seconds counting. PWV is measured by two oil filled the Acoustic Rolling Contact (ARC) transducers, which are mounted on the center sensor stand with the gamma system. These transducers measure the velocity of P-wave through the whole core and the pulse amplitude. MS is measured by the loop sensor of 100 mm diameter made by the Bartington Instruments Ltd. An oscillator circuit in the sensor produces a low intensity (approx. 80 A/m RMS) non-saturating, alternating magnetic field (0.565 kHz). MS was measured with 1 second. The measured raw data are shown in Fig. 4.2.4-1∼4. After the MSCL measurement, whole-core samples are cut into Working and Archive halves by a splitting devise and a nylon line. Fig. 4.2.4-1: MS raw data and color data (PC01; Guafo area). Fig. 4.2.4-2: MS raw data and color data (PC02; Off Taitao). Fig. 4.2.4-3: MS raw data and color data (PC03; Off Taitao). Fig. 4.2.4-4: MS raw data and color data (PC04; Off Chile). 4.2.5 Core color reflectance (CCR) (1) Personnel: Yuki Miyajima (Marine Works Japan Ltd.); miyajimay@mwj.co.jp (2) Objectives To understand characteristics of sediments such as lithology, redox condition, relative carbonate content, organic matter content and certain inorganic compounds, color reflectance was measured for split half sediments. (3) Measured Parameters There are different systems to quantify the color reference for soil and sediment measurements, the most common is the L*a*b* system, also referred to as the CIE (Commision International d’Eclairage) LAB system. It can be visualized as a cylindrical coordinate system in which the axis of the cylinder is the lightness variable L* ranging from 0% to 100%, and the radii are the chromaticity variables a* and b*. Variable a* is the green (negative) to red (positive) axis, and variable b* is the blue (negative) to yellow (positive) axis. Spectral data can be used to estimate the abundance of certain components of sediments. (4) Instruments and Methods Core color reference was measured by using the Konica Minolta CM-700d reference photo spectrometer using 400 to 700nm in wavelengths. This is a compact and hand-held instrument, and can measure spectral reflectance of sediment surface with a scope of 3 mm diameter. To ensure accuracy, the CM-700d was used with a double-beam feedback system, monitoring the illumination on the specimen at the time of measurement and automatically compensating for any changes in the intensity or spectral distribution of the light. The CM-700d has a switch that allows the specular component to be include (SCI) or excluded (SCE). We chose setting the switch to SCE. The SCE setting is the recommended mode of operation for sediments in which the light reflected at a certain angle (angle of specular reflection) is trapped and absorbed at the light trap position on the integration sphere. Calibrations are zero calibration and white calibration before the measurement of core samples. Zero calibration is carried out into the air. White calibration is carried out using the white calibration piece (CM-700d standard accessories) without crystal clear polyethylene wrap. The color of Archive half core was measured on every 1 cm through crystal clear polyethylene wrap. Measurement parameters are displayed Table 4.2.5-1. The measured raw data are summarized in Fig. 4.2.3-1∼4. Table 4.2.5-1: Measurement parameters. Instrument Konica Minolta Photospectrometer CM-700d Software Spectra Magic NX CM-S100w Ver.2.51 Illuminant d/8 (SCE) Light source D65 Viewing angle 10 degree Color system L*a*b* system 4.2.6 Core photograph (1) Personnel: Mika Yamaguchi (Marine Works Japan Ltd.); yamaguchim@mwj.co.jp (2) Objectives Photographs were taken to observe sedimentary structures of the cores. (3) Instruments and methods Each of Archive half core photographs were taken using a digital camera (Camera body: Nikon D90/ Lens: Nikon AF-NIKKOR 28 mm 1:1.8 D). When using the digital camera, shutter speed was 1/15 ~ 1/40 sec, F- number was 4.5~5.6, sensitivity was ISO 200. File format of raw data is JPEG. Details for settings were included on property of each file. 4.2.7 Visual Core Description (1) Personnel Frank Lamy (Alfred Wegener Institute); Frank.Lamy@awi.de Helge Arz (Ernst-Moritz-Arndt-University Greifswald); helge.arz@io-warnemuende.de (2) Summary Visual core description was made on the split surface of the archive half sections. The split surface was scraped using a plastic card to expose fresh surface. Lithological and sedimentological features were described in Fig. 4.2.7-1∼5 (detailed description for each section is in Appendix 1). Primary sediment lithologies were first described directly on the core and later confirmed/modified by a qualitative and quantitative microscopic examination of representatively taken smear slides (smear slide result table see in Appendix 1). We adopted the IODP- style nomenclature for lithological description (e.g., Mazzullo et al., 1988) with some modifications. Cores PC01 and PC02 were retrieved close to core locations of the MD159 cruise in 2007 (MD159 – PACHIDERME, IMAGES XV, 2007; cores MD07-3088 and MD07-3119, respectively) with the advantage that Siani et al. (2010) provides a detailed chronostratigraphic framework for core PC01 and the upper part of PC02 based on radiocarbon and tephrochronological data. Onboard GEOTEK measurement of the magnetic susceptibility and GRAPE density were used for a detailed correlation between PC01 and MD07-3088 used for establishing of a preliminary chronostratigraphy. Core PC01 consists in a fairly uniform succession of olive black to grayish olive nannofossil/diatom and silt bearing to silty clay (Fig. 4.2.7-1, 6). Magnetic susceptibility is generally quite low and the correlation to core MD07-3088 (Fig. 4.2.7-6∼7) suggests a basal age of 17.5 kyrs BP, thus covering most of the glacial Termination I and the Holocene. Further offshore, two piston cores of 13 and 17 m were retrieved at 2786 and 3067 m water depth, respectively (Station 03, core PC02 and Station 08, core PC03) from the Chile Rise showing a well-developed stratification in the seismic record. The cores are well comparable and consist of dark olive gray to grey silt- diatom- and occasionally nannofossil-bearing clay to clayey nannofossil ooze with some thin silt and sandy layers that become more frequent in the lower part of the cores and which could be ascribed mainly to turbididic deposits and perhaps also to tephra layers. In core PC03 magnetic susceptibility is low in the upper and the lowermost three meters characterizing sediment with an increased amount of biogenic components. Most of the core, however, consists of glacial clayey sediments with an alternating contribution of coarser grained siliciclastics. At about 9.1 m a prominent 15 cm thick brownisch tephra layer interrupts the normal sedimentation (Fig. 4.2.7- 8). The biogenic-rich basal three meters were deposited most probably during the last interglacial Marine Isotope Stage (MIS) 5 and the basal age of the core is suggested to be around 120-130 kyrs BP (Fig. 4.2.7-9). Core PC04 was cored in 3852 m water depth in the deeper Southeast Pacific south of the Chile Rise at (~50.8°S) ~200 nm off the Chilean coast. Sediment acoustic profiles from this region revealed well-stratified deposits with significantly increased acoustic penetration. With respect to major lithologies, the core is quite different from the shallower continental margin cores further to the northeast. Overlain by a yellowish brown foraminifera and diatom-bearing nannofossil ooze, dark olive to greenish gray clays dominate the sequence. The clay sequence is intercalated with lighter foram-bearing calcareous oozes, the base of which is commonly strongly bioturbated. Calcareous oozes are found at ~3- 4, 9-10, ~13, and 14.5-15.5 m. At 14.5-15.5 m the calcareous oozes consist of a compact, stiff, white nannofossil ooze (Fig. 4.2.7-10). The recovered sequence in PC04 is quite similar to those described in cores PS97/112-1 and 114-2 that were recovered during the RV Polarstern cruise PS97 in 2016 about 120 nm offshore Chile 4° further to the south (55°S) from a comparable water depth of ~3850 m (Expedition PS97 cruise report, 2016). The records of cores PC04 and PS97/114-2 correlate convincingly (Fig. 4.2.7-11). The tentative correlation to the Lisiecki & Rymo (2005) isotope stack and to the Antarctic climate records suggests that the core PC04 reaches back to the Marine Isotope Stage 12 (430 kyrs BP) and has an average sedimentation rate of about 4 cm/kyr. When all PC cores are compiled into one graph, an almost linear relationship between the average sedimentation rate and the distance to the Chilean coast becomes evident. This relationship mainly describes the diminishing influence to the west of the detrital sediment input from the glaciated southernmost Andes (Fig. 4.2.7-12). References: Kissel C. and cruise participants (2007): MD159 – PACHIDERME IMAGES XV Cruise report. IPEV, Les rapports de campagnes a` la mer, 83 pp. Lamy, F. and cruise participants (2016): The Expedition PS97 of the Research Vessel POLARSTERN to the Drake Passage in 2016. Reports on Polar and Marine Research 701, 157 pp. doi:10.2312/BzPM_0701_2016 Mazzullo, J., Meyer, A. and Kidd, R. (1988) New sediment classification scheme for the Ocean Drilling Program. Appendix I, In “Handbook for shipboard sedimentologists” eds. Mazzullo, J. and Graham, A. G., ODP Technical Note, 8, 44-63. Siani, G., Colin, C., Michel, E., Carel, M., Richter, T., Kissel, C., and Dewilde, F. (2010): Late Glacial to Holocene terrigenous sediment record in the Northern Patagonian margin: Paleoclimate implications, Palaeogeogr. Palaeocl., 297, 26–36. Fig. 4.2.7-1: Visual core description for PC01. Fig. 4.2.7-2: Visual core description for PC02. Fig. 4.2.7-3: Visual core description for PC03. Fig. 4.2.7-4: Visual core description for PC04. Fig. 4.2.7-5: Legend for core description. Fig. 4.2.7-6: Graph combining the GEOTEK magnetic susceptibility measurements on core PC01 with the smear slide examinations on the core. Fig. 4.2.7-7: Correlation of the magnetic susceptibility records of dated core MD07-3088 (Siani et al. 2010) and PC01 with PC01 sedimentation rates. Fig. 4.2.7-8: Graph combining the GEOTEK magnetic susceptibility measurements on core PC03 with the smear slide examinations on the core. Fig. 4.2.7-9: Correlation of the magnetic susceptibility records of cores PC01, PC02, and PC03 with approximate basal age and average sedimentation rates. Fig. 4.2.7-10: Graph combining the GEOTEK magnetic susceptibility measurements on core PC04 with the smear slide examinations on the core. Fig. 4.2.7-11: Correlation of the magnetic susceptibility and GRAPE density data of core PC04 and core PS97/114-2 on a common PS97/114-2 depth scale. Gray bars tentatively indicate the interglacial Marine Isotope Stages 1 to 11. Fig. 4.2.7-12: Close to linear relationship between the average sedimentation rates of cores PC01, PC02, PC03, and PC04 and their distance to the Chilean coast. 4.3 Dredge 4.3.1 Dredge System (1) Personnel Yusuke Sato (Marine Works Japan Co. Ltd); satoy@mwj.co.jp Ei Hatakeyama (Marine Works Japan Co. Ltd); hatakeyamae@mwj.co.jp Yohei Katayama (Marine Works Japan Co. Ltd); katayamay@mwj.co.jp (2) Objective Collection of seafloor rocks and sediments (3) Instruments and Methods The dredge sampler system used during MR16-09_Leg2 cruise is shown in Fig.4.1.3-1, showing the configuration of Transponder, Winch wire, Lead wire, Chain, Weight, Pipe dredge, Life wire, Fuse wire and Main Chain-bag Dredge. Fig. 4.1.3-1: Dredge system with a box-type dredge. Transponder: Transponder is an equipment that receives acoustic signals and automatically sends out another signal in reply. In this cruise, it is used to make sure the roughly position of the dredge sampler system in water. It was put on the winch wire in two cramps with special housing. Winch wire: Diameter of winch wire is 17mm. It is 0.983kg weight per one meter in water (i.e. about 983kg for 1,000m in the sea water) and having a 24.2t breaking force. Lead wire: This wire is prepared for protection against damage to the winch wire, jointed by shackles (3.15t SUS) and a swivel (5t). It is iron wire of 12mm diameter, 200m long and a 7.24t breaking force. Chain: Chain (19mm diameter, 5m long) is used to stabilize the dredge sampler and was jointed to the lead wire with a swivel (5t) and shackles (φ19). Weight(50kg per each): The weight is used to assure the dredge sampler is on the bottom as can be observed by the tension meter in the operation room, and linked by shackles (φ16) to the chain together with a swivel (1t), fuse wire (8mm diameter, 0.25m long) and life wire (10mm diameter, 1.7m long). Pipe dredge: Pipe dredge assumes the function as the backup of the main chain-bag dredge. This is linked as same as the weight. (Life wire is 1m long) Life wire (chain-bag): End of the life wire (10mm diameter, 7 m long) is connected parallel with fuse wire, and the other end is connected with the middle part of the chain-bag. In the case of fuse wire is broken by a big bite or anchoring, life wire works to prevent the dredge from lost, and keeps the samples in the box type bucket. Fuse wire: Fuse wire (8mm diameter, 0.25m long) is prepared to release the dredge from big bites that might damage the winch wire. It is jointed to the chain with a swivel (1t or 3t) and shackles in the main chain-bag dredge. Chain-bag dredge: The square type dredge consists of box type jaw (60*45 cm mouth, 60*27 cm throat), handle (26mm diameter, 85cm long) and steel chain-bag (6 mm diameter, 100cm long) with box type bucket (27*60*50cm) made from stainless steel (5mm thick). The bucket can recover all kinds of sediments on seafloor, it was jointed with shackles to the 0.25 m fuse wire. About details of wire diameter and breaking force are written in below. Diameter Breaking Force ———————— —————————————— 6mm 1.81t 8mm 3.22t 10mm 5.03t 12mm 7.24t (4) Operation note Operation of dredging was conducted on the basis of following strategies. i. Preparation We set the start and end point for dragging of the dredge system on the basis of the contour map. ii. The points should be checked before and during deploying the dredge system Carefully check on “no loose connections” between the main body, weight, pipe dredge, wires, and chain. Connect transponder to 50 m of the main wire. iii. Approaching to bottom Until reach the dredge system to about 100 m depth above the seafloor, the main wire should be rolled out 1.0 m/s. Keep stopping of wire-out about 3 min, and position and movement of transponder should be checked. Wire out restart by the speed of 0.3 m/s until dredge on bottom. iv. On bottom If we find that the position of transponder is just beneath of stern immediately before the dredge system on bottom, ship should be start to move to the end point in 0.5 knot. Reach of the dredge system to bottom should be identified on the basis of reduction of tension of the main wire. The main wire is NOT further rolled out after the dredge system on bottom. The speed of ship increase to 1.0 knot. If slight increasing of tension is identified, the speed of ship decrease to 0.5 knot, and several tens of meters (depend on inclinations of slope) of the main wire should be rolled out. Important point: speed of the dredge system should NOT be more than 1 knot. In the case of the main wire is rolled in, ship should keep position, and speed of wire is 0.3 m/s. v. Off bottom We can find out off bottom of the dredge system, if carefully watch the changing of tension of the main wire on the tension meter. The altitude of 200 or 250 m for transponder is the most important information to identify completely off bottom of the dredge system. The speed of wire-in should be 0.5 m/s just after off bottom, and increase to 1.0 m/s if altitude of transponder is more than 250 m. 4.3-2 Dredge result (1) Parsonnel Natsue Abe (JAMSTEC) Shiki Machida (JAMSTEC) Ryo Anma (Univ. of Tsukuba) Yuji Orihashi (The Univ. of Tokyo) (2) Introduction The Chile Triple Junction (CTJ; Figure 4.3-2-1) is located where subducting spreading centers and accompanying fracture zones of the Chile Ridge system meet with the South American plate. This area is tectonically unique in that the ridge subduction accompanies obduction of an ophiolite nearby (namely, the Taitao ophiolite), providing an excellent opportunity to study the magmatism involved in the ridge subduction processes on land. Our continuous effort toward understanding this magmatism, including the R/V Mirai MR08-06 cruise (see Abe, 2009; Harada, 2009), revealed that intensive fore-arc granite magmatism took place during the 6 Ma ridge subduction event (Anma et al., 2009) due to partial melting of the subducting oceanic crust under garnet-free conditions (Kon et al., 2013) to produce I-type granites (Shin et al., 2015), sediments subducted along a fracture zone were incorporated into S-type magmatism in the fore-arc region (Anma and Orihashi, 2013; Shin et al., 2015). Based on these, we planned new dredge sampling for the MR16- 09 cruise. Fig. 4-3-2-1: Large area map around survey area. (3) Objective The purpose of the dredge sampling in the CTJ area is to collect rock/sediment samples that help to understand solid earth recycling processes occurring/occurred due to subduction of the Chile Ridge system. Target rocks for the dredge operations are 1) igneous rocks distributed in the fore-arc region, 2) MORBs from the Segment 1 of the Chile ridge system and fracture zones, 3) rocks comprising seamounts nearby the subducting Chile Ridge. The dredge in the fore-arc region aims to find unknown igneous activities that are equivalent to the magmatism observed in the Taitao ohiolite-granite complex (Shin et al., 2015). The dredge of MORBs and seamount rocks aims to understand compositions of input materials that subduct and eventually melt to form arc magmas at deeper part of the ridge subduction zone. (4) Results Three dredge operations (D11~D13) were performed for the input rocks (MORBs and seamount). The positions of each dredge hauls are listed in the Table 4-3-2-1. Detail description of samples and photo image, and the table of all sample list are attached as Appendix. D11 to the seamount in the west of Segment 1 recovered pebbles of sub-rounded chert and sandstone, supposedly drop-stones, embedded in mud. Thus, the frank of the seamount was covered by a thick sediment. D12 operation to collect MORB from the Segment 1 was very successful and recovered sum of ~120 kg of basalts partly with quenched glassy rinds. In contrast, D13 to a neighboring mound to the D12 site recovered only few small pieces of volcanic glass (perhaps contamination of D12 dredge) in mud. Furthermore, a dredge operation was planned to collect altered basalts from the fracture zone between Segment 1 and Segment 2 spreading ridges. However, due mostly to wind and current of undesirable direction, this operation was canceled. Four dredge operations (D14~D17) were performed to find unknown igneous activities in the accretionary complex developed around 47°47’S. We initially planed for dredging nearby the Taitao peninsular for the investigation of the unknown igneous activities, but this attempt was abandoned due to rejection of applied permission for the operation in the Chilean water. As a contingency plan, this area was chosen to find igneous activities due to a ridge subduction event that took place ~14 Ma ago. All dredge operations were successful and we recovered siltstones and sandstones with gravels and conglomerates with different degree of consolidation. The degree of consolidation was measured using a needle penetration tester onboard. The sedimentary rocks from the seaward ridge (D14) were variously consolidated and contain chaotic rocks and various deformation structures including composite foliation and folds developed mainly in mudstones, and calcite veins. Rocks from a landward ridge (D15~17) contain turbidite with various grain size, sedimentary structures, and different degree of consolidation. No calcite vein was observed and deformation texture was less developed comparing to the seaward ridge. These sedimentary rocks will be further examined to understand development of new accretionary prism after the ridge subduction event. A piece of granite was recovered from D16 operation. Further investigation will be made to determine the age of this rock. (5) References Abe, N. (2009) MIRAI Cruise Report: MR08-06 Leg1, JAMSTEC Cruise Report, 140 p. Anma, R., Armstrong, R., Orihashi, Y., Ike, S., Shin, K-C., Kon, Y., Komiya, T., Ota, T., Kagashima, S., Shibuya, T., Yamamoto, S., Veloso, E. E., Fannin, M. and Herve, F. (2009) Are the Taitao granites formed due to subduction of the Chile ridge? Lithos, 113, 246-258. Anma, R. and Orihashi, Y. (2013) Shallow-depth melt eduction due to ridge subduction: LA-ICPMS U-Pb igneous and detrital zircon ages from the Chile Triple Junction and the Taitao Peninsula, Chilean Patagonia. Geochemical Journal, 47, 149-165. Harada, N. (2009) MIRAI Cruise Report: MR08-06 Legs. 2 and 3, JAMSTEC Cruise Report, 181 p. Kon, Y., Komiya, T., Anma, R., Hirata, T., Shibuya, T., Yamamoto, S. and Maruyama, S. (2013) Petrogenesis of the ridge subduction-related granitoids from the Taitao Peninsula, Chile Triple Junction area. Geochemical Journal, 47, 167-183. Shin, K-C., Anma, R., Nakano, T., Orihashi, Y. and Ike, S. (2015) The Taitao ophiolite-granite complex, Chile: Emplacement of ridge-trench intersection oceanic lithosphere on land and origin of calc-alkaline I-type granites. Episodes, 38, 285-299. Table 4-3-1: Position, depth, tension and hauling time information for each dredge haul during MR16-09 Leg2. MR16-09 Leg2 Dredge summary Depth (m) On the bottom Off the bottom ——————————————— Tension Date Dredge Location —————————————————————————————————————————————————— —————————————————————————————————————————————————— On the Off the max Survey (UTC) number Lat.(SOQ*) Lon.(SOQ*) Lat.{SOJ) Lon .{SOJ) Lat.(SOQ*) Lon.( SOQ*) Lat.(SOJ) Lon.(SOJ) bottom Bottom (t) time ————————— —————— —————————— ——————————— ——————————— ——————————— ——————————— ——————————— ——————————— ——————————— ——————————— —————— —————— ——————— ——————— 2017/1/23 Dll Off Taitao 46-l0.0787S 76-l6.3538W 46-10.12l9S 76-16.4333W 46-10.0917S 76-17.0023W 46-10.1550S 76-17.2010W 2,574 2,377 2.3 lhl0min 2017/1/24 D12 Off Taitao 45-52.45l4S 75-58.7050W 45-52.4510S 75-58.8027W 45-52.4599S 75-58.8688W 45-52.4718S 75-59.0717W 3,227 3,307 5.6 32min 2017/1/24 D13 Off Taitao 45-52.6695S 75-59.7638W 45-52.6187S 75-59.7023W 45-52.5500S 75-59.5170W 45-52.4482S 75-59.3372W 3,312 3,281 3.0 40min 2017/1/26 D14 Off Byron 47-46.3587S 76-25.6057W 47-46.3044S 76-25.6099W 47-46.3046S 76-24.8910W 47-46.2416S 76-24.8186W 3,080 2,658 4.3 lh35min 2017/1/26 D15 Off Byron 47-47.5231S 76-02.8022W 47-47.4710S 76-02.81l4W 47-47.3277S 76-02.6454W 47-47.2650S 76-02.6813W 1,930 1,755 4.8 lh0min 2017/1/28 D16 Off Byron 47-47.4854S 76-0l.8054W 47-47.4266S 76-01.8181W 47-47.2096S 76-0l.5343W 47-47.1330S 76-0l.5307W 1,831 1,511 2.6 lhllmin 2017/1/28 D17 Off Byron 47-47.2193S 76-02.8223W 47-47.1944S 76-02.6611W 47-46.9474S 76-02.5245W 47-46.8179S 76-02.5215W 1,656 1,435 3.0 lh2min *SOQ = Transponder's position, SOJ = Ship's position 4.4 Biological Sample Zooplankton: Rationale and Methods for Sample Collection (1) Personnel: Prof. Leonardo Castro (COPAS Sur Austral Center, Universidad de Concepción, Chile. (2) Rationale During the last years, the use of carbon and nitrogen isotopes has started to be widely utilized to study the structure of the food webs in marine ecosystems. Because enrichment of stable isotopes occurs along the trophic web, stable isotopes such as of carbon (13C) may be used to trace the original carbon source at the base of the web or, as in the case of nitrogen (15N) may be utilized as indicator of the trophic position organisms reaches along the web (Vander Zanden & Rasmussen 1999, Vander Zanden et al. 2001, Bode et al. 2003, 2007; Vargas et al. 2011, Montecinos et al. 2016). The information available on the marine pelagic community at the Cabo de Hornos Current off the Chilean Patagonia, on its major functional components and the trophic web structure, are very limited. This area, where water masses of different origin (SASW; ESSW, AAIW and EW) (Sievers & Silva 2006, Silva et al. 1997, 1998) converge in a narrow zone both in the horizontal and vertical domain, is expected to contain epi- and mesopelagic organism of diverse origin as well as trophic webs that channelize organic carbon from different sources at different depths. Since some of the micronekton (i.e. myctophid fishes) and mesozooplankton components (i.e. euphausiids) may change their depth of residence during diel vertical migrations or as they develop, changes also in the carbon signature and trophic position of these organisms are also expected to be visualized along the water column. In the present study, utilizing mesozooplankton samples collected from different depths along the Cabo de Hornos Current, the structure and food web of the epi- and mesopelagic plankton community is assessed by means of stable isotope analyses of the key species zooplankton (and ichthyoplankton) and major functional groups. In principle, differences in the carbon and nitrogen signals (δ13C; δ15N) are expected locally at organisms residing the surface layer according to the influence of major water inputs from the continent (e.g. off the Boca del Guafo, Golfo de Penas; Estuarine Waters). Secondarily, differences are expected also in the vertical plane according to the most common residence layers of the major zooplankton/ichtyoplankton taxa as a result of the influence of the trophic webs associated to the major waters masses present in the area at different depths (SASW; ESSW and AAIW). This information, besides describing for the first time the complex structure of the zooplankton community, will provide insights on the potential importance of the alloctonous material ingress (organic carbon from the continent) to the Cabo de Hornos Current to subsidize the pelagic trophic webs of this Patagonian offshore area. (3) Methods Field work. During the MIRAI Cruise MR 16-09 Leg 2, stratified zooplankton samples were collected at 8 bio-oceanographic stations (Table 1). At 7 of these stations, stratified zooplankton samples were collected through oblique tows with a Tucket Trawl net (1m2 mouth opening, 300um mesh, equipped with a GO flowmeter) from 3 (0-50m; 50-400 m; 400-600m) or more strata (up to 6 strata; maximum depth 600m) at day time hours. At an additional station, and due to harsh weather conditions, the stratified oblique sampling was switched to vertical tows with a WP2 net (60 cm mouth diameter, 300um mesh) from 3 depth ranges: 0-50m, 0-400m, 0-600m. On board, the zooplankton samples were splitted and one fraction was preserved in formaline 5% for zooplankton identification and counting, and another was frozen down to -80°C for stable isotope (δ13C; δ15N) analyses. Table 1: Summary of zooplankton samples collected during the MIRAI Cruise MR 16-09 - Leg 2 along the Cabo de Hornos Current, showing station number, type of net utilized, sampled depth range, and number of subsamples preserved and frozen. Sampled Subsamples Station Sampling Depth Range Formaline Frozen Total gear (m) 10% -80°C subsamples ——————— ———————————— ——————————— —————————— —————— —————————— 1 Tucker trawl 0 - 400 1 1 2 400 - 50 1 1 2 50 - 0 1 1 2 0 - 600 1 1 2 600 - 400 1 1 2 400 - 0 1 1 2 4 Tucker trawl 0 - 400 1 1 2 400 - 50 1 1 2 50 - 0 1 1 2 8 Tucker trawl 0 - 400 1 0 1 400 - 50 1 1 2 50 - 0 1 1 2 0 - 600 1 0 1 600 - 400 1 1 2 7 Tucker trawl 0 - 400 1 0 1 400 - 50 1 1 2 50 - 0 1 1 2 9 Tucker trawl 0 - 400 1 0 1 400 - 50 1 0 1 50 - 0 1 0 1 10 Tucker trawl 0 - 400 1 0 1 400 - 50 1 1 2 50 - 0 1 1 2 600 - 400 1 1 2 11B Tucker trawl 0 - 400 1 1 2 400 - 50 1 1 2 50 - 0 1 1 2 600 - 400 1 1 2 12B WP2 0 - 600 1 0 1 0 - 400 1 0 1 0 - 50 1 0 1 —————————————————————————————————————————————————————————————————— 8 7 Tucker 31 samples 31 21 52 stations + 1 WP2 References Bode, A., Carrera, P., Lens, S., 2003. The pelagic food web in the upwelling ecosystem of Galicia (NW Spain) during spring: natural abundance of stable carbon and nitrogen isotopes. ICES Journal of Marine Science, 60: 11-22. Bode, A., Alvarez-Ossorio, M.T., Cunha, M.E., Garrido, S., Peleteiro, J.B., Porteiro, C., Valdes, L., Varela, M., 2007. Stable nitrogen isotope studies of the pelagic food web on the Atlantic shelf of the Iberian Peninsula. Progress in Oceanography, 74, 115-131. Montecinos S., L R. Castro & S Neira. 2016. Stable isotope (δ13C and δ15N) and trophic position of Patagonian sprat (Sprattus fuegensis) from the Northern Chilean Patagonia. Fisheries Research 179 (2016) 139–147. Sievers H.A. & N Silva. 2006. Masas de agus y circulación en los canales y fiordos australes. En N. Silva y S Palma (Eds),"Avances del conocimiento oceanográfico de las aguas interiores chilenas: Puerto Mont a cabo de Hornos". Comité Oceanográfico Nacional. P Universidad Católica de Valparaíso. Pp. 53-58. Silva N, C Calvete & H. Sievers. 1997. Características oceanográficas físicas y químicas de canales australes chilenos entre Puerto Montt y Laguna San Rafael (Crucero Cimar-Fiordo l). Ciencia y Tecnología del Mar 20: 23-106 Silva.N, C Calvete & H. Sievers. 1998. Masas de agua y circulación general para algunos canales autrales entre Puerto Montt y Laguna San Rafael, Chile (Crucero CIMAR Fiordo l). Ciencia y Tecnología del Mar 21. 17-48. Vander Zanden, M.J., Rasmussen, J.B., 1999. Primary consumer delta C-13 and delta N-15 and the trophic position of aquatic consumers. Ecology, 80, 1395-1404. Vander Zanden, M.J., Rasmussen, J.B., 2001. Variation in delta N-15 and delta C-13 trophic fractionation: Implications for aquatic food web studies. Limnology and Oceanography, 46, 2061-2066. Vargas, C.A., Martinez, R.A., San Martin, V., Aguayo, M., Silva, N., Torres, R., 2011. Allochthonous subsidies of organic matter across a lake-river-fjord landscape in the Chilean Patagonia: Implications for marine zooplankton in inner fjord areas. Continental Shelf Research, 31, 187-201. 4.5 Suspended Particles (1) Personnel Humberto E. Gonzalez and Eduardo Menschel (Universidad Austral de Chile, Valdivia and FONDAP-IDEAL center, Valdivia and Punta Arenas, Chile) (2) Sampling and scientific motivation Two types of samples were collected: 1) Particulate Organic Carbon (POC) Methods: From 1.0 to 2.5 Lt of water were filtrated through a pre- combusted glass fiber filters (Whatman GF/F). The filters were stored frozen and at the laboratory were decarbonated (using HCl2 acid) and dried (at 50ºC overnight). The filter were sent to the University of California at Davis for C and N elemental composition and natural isotopes analysis. Scientific relevance: The POC constituted an important component of the carbon pool in the ocean and a key component of the carbon biogeochemical cycle (i. e. carbon export to the deep sea). It is a relevant proxy of the food resources available to be channeled through the microbial and particulate food webs in the ocean. In addition, the natural isotope signature can give us insights about the precedence (origin) of this POC. 2) Microzooplankton (µzoo) composition and abundance: Methods: From 7.0 to 12.0 Lt of water were filtrated through a 20 µm nitex sieve and resuspended in a final volume of ca. 300 ml. These samples were preserved with buffered lugol to further analysis at the laboratory. Scientific relevance: The µzoo are an important component of the heterotrophic functional groups of the plankton, especially in open waters. Some of these groups, such as foraminifers, radiolarians, can be used as paleoceanographic conditions. Almost no information on POC and µzoo from the deep ocean side of the eastern south Pacific are available. The analysis of these samples would contribute to fill the gap on the knowledge of the quantity and quality of these components. Station 1 21 Jan. 2017 Position (44º17S 75º36W) Max. Depth = 1928 m ————————————————————————————————————————————————————————————————————————— Sampling Filter Water Volume Water Volume depth (Nº) Filtrated for filtrated for (m) POC (Lt) µzoo (Lt) ——————————— —————— ————————————— ————————————— 0 135 1 10 10 552 1 7 25 32 1 7,5 50 343 1,5 7 100 79 2 7,5 700 344 2 7 1918 (B-10) 252 2 8 Station 4 24 Jan. 2017 Position (46º08S 76º04W) Depth = 2400 m time 00:05 hr, ————————————————————————————————————————————————————————————————————————— Sampling Filter Water Volume Water Volume depth (Nº) Filtrated for filtrated for (m) POC (Lt) µzoo (Lt) ——————————— —————— ————————————— ————————————— 0 307 1 10 10 30 1 10 25 162 1 10 50 166 1,5 10 100 169 2 10 300 317 2 10 700 177 2,5 7 1918 (B-10) 178 2,5 10 Station 7 28 Jan. 2017 Position (47º47,7S 76º02,6W) Depth = 2000 m time 05:30 hr, ————————————————————————————————————————————————————————————————————————— Sampling Filter Water Volume Water Volume depth (Nº) Filtrated for filtrated for (m) POC (Lt) µzoo (Lt) ——————————— —————— ————————————— ————————————— 0 335 1 11 10 173 1 11 25 160 1 11,35 50 412 1,5 10 100 251 2 10,2 300 182 2,5 9,9 500 181 2,5 9,95 700 180 2,5 7,1 1990 (B-10) 179 2,55 9,3 Station 9 29 Jan 2017 Position (48º23,5S 76º28,0W) Depth = 1800 m time 10:00 hr, ————————————————————————————————————————————————————————————————————————— Sampling Filter Water Volume Water Volume depth (Nº) Filtrated for filtrated for (m) POC (Lt) µzoo (Lt) ——————————— —————— ————————————— ————————————— 0 31 1 12,6 10 167 1 10,85 25 174 1 10,1 50 175 1,6 11,3 100 358 2 10,6 300 161 2,55 9,9 500 176 2,6 9 700 155 2,5 7,6 1790 (B-10) 329 2,55 10,6 Station 10 31 Jan. 2017 Position (50º48,3715S 79º07,096W) Depth = 3851 m time 05:30 hr, ————————————————————————————————————————————————————————————————————————— Sampling Filter Water Volume Water Volume depth (Nº) Filtrated for filtrated for (m) POC (Lt) µzoo (Lt) ——————————— —————— ————————————— ————————————— 0 140 1,5 10,9 10 328 1 11,1 25 159 1,5 11,4 50 60 1,6 10,1 100 137 2 8,6 300 138 2,5 11.4 500 139 2,5 9,1 700 141 2,5 9,8 3841 (B-10) 39 2,5 10,15 Station 12B 02 Feb. 2017 Position (54º20,09S 74º38,187W) Depth = 2400 m time 08:00 hr, ————————————————————————————————————————————————————————————————————————— Sampling Filter Water Volume Water Volume depth (Nº) Filtrated for filtrated for (m) POC (Lt) µzoo (Lt) ——————————— —————— ————————————— ————————————— 0 168 1 12,1 10 20 1 11,1 25 59 1 7,85 50 322 1,5 11,1 100 61 2 10 300 62 2,7 6,8 500 63 2,5 10,4 700 19 2,5 7,65 2390 (B-10) 18 2,5 9,8 Station 11B 03 Feb. 2017 Position (53º00,08S 75º29,08W) Depth = 1762 m time 01:10 hr, ————————————————————————————————————————————————————————————————————————— Sampling Filter Water Volume Water Volume depth (Nº) Filtrated for filtrated for (m) POC (Lt) µzoo (Lt) ——————————— —————— ————————————— ————————————— 0 142 1 11 10 146 1 10,5 25 145 1 10,3 50 144 2 10,1 100 64 2 10 300 89 2,5 10 500 147 2,5 10,6 700 34 2,5 7,6 1752 (B-10) 133 2,5 10 Station 11A 03 Feb. 2017 Position (52º19,0681S 75º56,9148W) Depth = 1880 m time 17:40 hr, ————————————————————————————————————————————————————————————————————————— Sampling Filter Water Volume Water Volume depth (Nº) Filtrated for filtrated for (m) POC (Lt) µzoo (Lt) ——————————— —————— ————————————— ————————————— 0 131 1 11,8 10 383 1 11,55 25 37 1 10,5 50 129 1 10,6 100 125 2 10,4 300 134 2,5 10,65 500 1 2,5 10,95 700 325 2,5 10,5 1870 (B-10) 36 2,5 10,45 4.6 Physiological Characteristics of Phytoplankton Assemblages in the Southern Patagonia Pacific Margin Waters J.L. Iriarte* and T. Shiozaki† * Centro Investigación Dinámica de Ecosistemas Marinos de Altas Latitudes – IDEAL – Universidad Austral de Chile. COPAS-Sur Austral, Centro de Investigación Oceanográfica en el Pacífico Sur-Oriental (COPAS-Sur Austral), Universidad de Concepción, Chile † Research and Development Center for Global Change, Japan Agency for Marine-Earth Science and Technology – JAMSTEC, Japan Introduction High-latitude ecosystems are immersed in environmental regimes that may strongly constrain biological productivity. Rhythms and rates of primary production in these highly seasonal environments depend to a large extent on the timing of nutrient supply and light availability for primary producers. In the fjords and channels of southern Chile, the interaction between oceanic water and freshwater from multiple sources (rivers, surface runoff, snow/glacier melting, precipitation) produces strong vertical and horizontal gradients in salinity, density, inorganic nutrient ratios and light availability. These gradients, and their seasonal and inter-annual changes, may affect both the biomass and composition of phytoplankton assemblages, and ultimately shape the spatial-temporal patterns of carbon fixation, organic matter fluxes, and biogeochemical balances in this region. Vertical mixing and the exchange of nutrients among the low-salinity, low nutrient and turbid surface layer and the more saline sub-surface layer are the main drivers of spring pulses in primary production and autotrophic biomass. The concentrations of inorganic nutrients show a strongly seasonal signal, with high nitrate and orthophosphate during winter, and lower values during spring, presumably caused by a sharp increase in primary productivity when light availability in near-surface waters increases (Iriarte et al 2007; González et al 2011). Beyond the changes in concentrations of macro and micronutrients, however, changes in freshwater regimes may modify the inorganic chemistry of euphotic-zone waters. In addition, increasing discharges of freshwater from glacier melting and river runoff may alter the acid-base chemistry of near- surface waters, thereby establishing spatial gradients in alkalinity that may in turn determine shifts in phytoplankton composition (e.g. from cyanobacteria/chlorophytes to Diatoms/Dinoflagellates; Chakraborty et al 2011) and productivity (Shi et al 2009). Specifically, combine abiotic factors (e.g. temperature, salinity, Fe, light) may play important role in defining the physiological state of phytoplankton, by inhibitory effects on physiological processes on phytoplankton cells (e.g. respiratory activity). Adaptation mechanisms at cellular level (photosystems I and II, photoprotective pigments) could impact the photochemical efficiency of photosynthesis and thus result in reduced growth rates and photosynthesis efficiency (PS II, Fv/Fm). Basically, our conceptual model would work in the following steps: the presence of high(low) driver (freshwater, wind stress) causes the formation of deep(shallow) mixed layer and pycnocline depth, leading to a rapid water column fluctuation in irradiance (high near surface and low near the pycnocline), which may impinge a great stress on the physiological dynamics of phytoplankton. The studied area is the large continental shelf of Patagonia (Fig. 1), influenced by freshwater from largest adjacent rivers discharging freshwater. The interplay between freshwater and oceanic water types strongly interact with nutrients supply and may determine the magnitude of phytoplankton biomass and composition. We combine the continuous in situ profiling of fluorescence with oceanographic variables in summer to estimate photosynthetic efficiency, phytoplankton biomass and composition, along with observations of inorganic nutrients, in the continental shelf to address a main question on to what extent the spatial changes in near surface water chemistry may affect phytoplankton community properties in oceanic Patagonian waters. Figure 4.6-1: Autotrophic biomass (as Chlorophyll-a, µg L-1) vertical distribution for phytoplankton communities at 8 stations, along the Patagonian shelf, January-February 2017. Depth interval: 0 – 100 m. Material and Methods For the first time, we studied physiological features of phytoplankton assemblages in the Patagonian oceanic surface waters using a real-time Fast Repetition Rate Fluorometer (FRRf, Chelsea Technology Group, UK) at 12 stations during austral summer (19 January – 5 February 2017). At each station FRRf equipped with a 20 m cable was deployed in profiling mode with a approximate speed of 0.5 m s-1. With the exception of one station (11B, 21:30 h)), all measurements were done during the daylight between 9:30 to 15:30 h. Fluorescence readings were corrected for background fluorescence signals using filtered seawater previously collected at 10 m depth. All the FRRf deployment were carried out from stern of the vessel. This is essentially a measure of the quantum efficiency of photosystem II and provides an indication of cell health. All these variables and photosynthetic coefficients would give information on the effect of vertical stratification (pycnocline, light, nutricline) on the distribution of nPS II during different stations along Patagonia. In addition, it would be expected to find a significant correlation between photosynthetic efficiency fluorescence-based and in situ autotrophic biomass (as chlorophyll-a) and primary productivity determined by 13C method in Patagonian waters. Results and Discussion Along the shelf transect the highest chlorophyll-a concentrations were observed in the northern area (Sta., 6, 7, 9) at the base of the pycnocline in the upper layer (0 – 25 m) with a mean value of 2.63 µg L-1 (range: 1.64 – 3.76 µg L-1) (Fig. 4.6-1). These were associate with the stratified upper part of the water column (< 30 m) and coincided with relatively low salinities (32.75 – 33.35). For the southern stations (Sta., 11, 12), maximum chlorophyll-a values were lower than 1.79 µg L-1 (mean: 1.01 µg L-1) in the upper 25 m. Figure 4.6-2: Vertical distribution of quantum efficiencies of photochemistry in PSII (F’q/F’m) and functional absorption cross section of photosystem II (σ’PSII: Å2 m-2) for phytoplankton communities under ambient light at 13 stations, along the Patagonian shelf, January-February 2017, were obtained by a Fast Repetition Rate Fluorometer (FRRf). Depth interval: 0.5 – 20 m. Figure 4.6-3: Horizontal distribution of quantum efficiencies of photochemistry in PSII (F’q/F’m) and functional absorption cross section of photosystem II (σ’PSII: Å2 m-2; values*100) for phytoplankton communities under ambient light at 8 stations, along the Patagonian shelf, January- February 2017, were obtained by a Fast Repetition Rate Fluorometer (FRRf). Depth interval: 0.5 – 20 m. In general, the effective photochemical efficiency of PSII (F’q/F’m) was low and ranged between 0.081 to 0.497 (median = 0.308, 25% percentile = 0.22, 75% percentile = 0.384), increasing from surface to depth (20 m) at all stations (Y = 0,249 + 0.0054*depth, p = 0.0001, N = 1025) (Fig. 4.6-2). In the northern area (Sta., 2, 6,) F’q/F’m values increased with depth, attaining values of 0.3 between 5 to 10 m. At southern stations (Sta., 11, 12) 0.3 - 0.45 quantum efficiencies were observed from 5 to 20 m range depth. It seems to be influenced by the low surface salinities, with low values (>0.3) observed in the upper 5 m, while higher than 0.3 quantum efficiency deeper than 5 m were observed at southern stations characterized by deeper mixed layer. While the functional absorption cross section of photosystem II under ambient light (σ’PSII) showed a homogeneous vertical distribution at most of the stations or slightly increasing with depth (Y = 4.138 + 0.0226*depth, p = 0.0001, N = 1004) (range = 47 – 676 Å2 m-2; median = 442, 25% percentile = 220, 75% percentile = 384) (Fig. 4.6-2) and positive associated to quantum efficiency (Fig. 4.6-3). The preliminary results suggest us that the phytoplankton assemblages were adapted at lower irradiance in the upper 20 m depth. It was interesting to note that at stations 7 and 9, values higher than 500 Å2 m-2 functional were observed near surface and well correlated with chorophyll-a biomass. References Chakraborty P., T. Acharyya, P.V. Raghunadh Babu & D. Bandhyopadhyay. 2011. Impact of salinity and pH on phytoplankton community in a tropical freshwater system: an investigation with pigment analyses by HPLC. Journal of Environmental Monitoring. 13:614-620. Iriarte J.L., González H.E., Liu K.K., Rivas C. and Valenzuela C. 2007. Spatial and temporal variability of chlorophyll and primary productivity in surface waters of southern Chile (41.5–43°S). Estuarine Coastal and Shelf Science 74, 471–480. González, H.E., Castro, L., Daneri, G., Iriarte, J.L., Silva, N., Vargas, C., Giesecke, R., Sánchez N., 2011. Seasonal plankton variability in Chilean Patagonia fjords: carbon flow through the pelagic food web of the Aysen Fjord and plankton dynamics in the Moraleda Channel basin. Continental Shelf Research 31, 225-243. Shi D., Xu, Y., F.M.M Morel. 2009. Effects of the pH/pCO2 control method on medium chemistry and phytoplankton growth. Biogeosciences, 6:1199- 1207 4.7 CTDO2 Measurements May 14, 2017 (1) Personnel Hiroshi Uchida (JAMSTEC) Rei Ito (MWJ) Sonoka Tanihara (MWJ) Kenichi Katayama (MWJ) Shungo Oshitani (MWJ) Rio Kobayashi (MWJ) Michinari Sunamura (The University of Tokyo) (CDOM measurement) (2) Winch arrangements The CTD package was deployed by using 4.5 Ton Traction Winch System (Dynacon, Inc., Bryan, Texas, USA), which was renewed on the R/V Mirai in April 2014 (e.g. Fukasawa et al., 2004). Primary system components include a complete CTD Traction Winch System with up to 9000 m of 9.53 mm armored cable (Rochester Wire & Cable, LLC, Culpeper, Virginia, USA). (3) Overview of the equipment The CTD system was SBE 911plus system (Sea-Bird Electronics, Inc., Bellevue, Washington, USA). The SBE 911plus system controls 36-position SBE 32 Carousel Water Sampler. The Carousel accepts 12- litre Niskin-X water sample bottles (General Oceanics, Inc., Miami, Florida, USA). The SBE 9plus was mounted horizontally in a 36-position carousel frame. SBE’s temperature (SBE 3) and conductivity (SBE 4) sensor modules were used with the SBE 9plus underwater unit. The pressure sensor is mounted in the main housing of the underwater unit and is ported to outside through the oil-filled plastic capillary tube. A modular unit of underwater housing pump (SBE 5T) flushes water through sensor tubing at a constant rate independent of the CTD’s motion, and pumping rate (3000 rpm) remain nearly constant over the entire input voltage range of 12-18 volts DC. Flow speed of pumped water in standard TC duct is about 2.4 m/s. Two sets of temperature and conductivity modules were used. An SBE’s dissolved oxygen sensor (SBE43) was placed between the primary conductivity sensor and the pump module. Auxiliary sensors, a Deep Ocean Standards Thermometer (SBE 35), an altimeter (PSA-916T; Teledyne Benthos, Inc., North Falmous, Massachusetts, USA), an oxygen optodes (RINKO-III; JFE Advantech Co., Ltd, Kobe Hyogo, Japan), a fluorometers (Seapoint sensors, Inc., Kingston, New Hampshire, USA), a transmissometer (C-Star Transmissometer; WET Labs, Inc., Philomath, Oregon, USA), a turbidity meter (Seapoint Sensors, Inc., Exeter, New Hampshire, USA), a Photosynthetically Active Radiation (PAR) sensor (Satlantic, LP, Halifax, Nova Scotia, Canada), and a colored dissolved organic matter (ECO FL CDOM, WET Labs, Inc., Philomath, Oregon, USA) were also used with the SBE 9plus underwater unit. To minimize rotation of the CTD package, a heavy stainless frame (total weight of the CTD package without sea water in the bottles is about 1000 kg) was used with an aluminum plate (54 × 90 cm). Summary of the system used in this cruise 36-position Carousel system Deck unit: SBE 11plus, S/N 11P54451-0872 Under water unit: SBE 9plus, S/N 09P21746-0575 (79492) Temperature sensor: SBE 3, S/N 031525 (primary) SBE 3plus, S/N 03P4421 (secondary) Conductivity sensor: SBE 4, S/N 042435 (primary) SBE 4, S/N 041088 (secondary) Oxygen sensor: SBE 43, S/N 432471 JFE Advantech RINKO-III, S/N 0024 (foil batch no. 144002A) Pump: SBE 5T, S/N 054595 (primary) SBE 5T, S/N 053293 (secondary) Altimeter: PSA-916T, S/N 1157 Deep Ocean Standards Thermometer: SBE 35, S/N 0045 Fluorometer: Seapoint Sensors, Inc., S/N 3618 (measurement range: 0-15 µg/L) (Gain: 10X) Turbidity meter: Seapoint Sensors, Inc., S/N 14953 (measurement range: 0-500 FTU) (Gain: 5X) for leg 2 (measurement range: 0-25 FTU) (Gain: 100X) for leg 3 Transmissometer: C-Star, S/N CST-1726DR PAR: Satlantic LP, S/N 1025 CDOM: ECO FL CDOM, S/N FLCDRTD-2014 (measurement range: 0-500 ppb) Carousel Water Sampler: SBE 32, S/N 3254451-0826 Water sample bottle: 12-litre Niskin-X model 1010X (no TEFLON coating) General Oceanics, Inc., Miami, Florida, USA, (4) Pre-cruise calibration i. Pressure The Paroscientific series 4000 Digiquartz high pressure transducer (Model 415K: Paroscientific, Inc., Redmond, Washington, USA) uses a quartz crystal resonator whose frequency of oscillation varies with pressure induced stress with 0.01 per million of resolution over the absolute pressure range of 0 to 15000 psia (0 to 10332 dbar). Also, a quartz crystal temperature signal is used to compensate for a wide range of temperature changes at the time of an observation. The pressure sensor has a nominal accuracy of 0.015 % FS (1.5 dbar), typical stability of 0.0015 % FS/month (0.15 dbar/month), and resolution of 0.001 % FS (0.1 dbar). Since the pressure sensor measures the absolute value, it inherently includes atmospheric pressure (about 14.7 psi). SEASOFT subtracts 14.7 psi from computed pressure automatically. Pre-cruise sensor calibrations for linearization were performed at SBE, Inc. The time drift of the pressure sensor is adjusted by periodic recertification corrections against an electronic dead-weight tester (Model E-DWT-H, S/N 181, Fluke Co, Phoenix, Arizona, USA, Calibrated on 3 April 2016 at Ohte Giken, Inc., Tsukuba, Ibaraki, Japan). The corrections are performed at JAMSTEC, Yokosuka, Kanagawa, Japan by Marine Works Japan Ltd. (MWJ), Yokohama, Kanagawa, Japan, usually once in a year in order to monitor sensor time drift and linearity. S/N 0575, 13 April 2016 slope = 0.99982448 offset = 2.98685 ii. Temperature (SBE 3) The temperature sensing element is a glass-coated thermistor bead in a stainless steel tube, providing a pressure-free measurement at depths up to 10500 (6800) m by titanium (aluminum) housing. The SBE 3 thermometer has a nominal accuracy of 1 mK, typical stability of 0.2 mK/month, and resolution of 0.2 mK at 24 samples per second. The premium temperature sensor, SBE 3plus, is a more rigorously tested and calibrated version of standard temperature sensor (SBE 3). Pre-cruise sensor calibrations were performed at SBE, Inc. S/N 031525, 7 May 2016 S/N 03P4421, 7 May 2016 iii. Conductivity (SBE 4) The flow-through conductivity sensing element is a glass tube (cell) with three platinum electrodes to provide in-situ measurements at depths up to 10500 (6800) m by titanium (aluminum) housing. The SBE 4 has a nominal accuracy of 0.0003 S/m, typical stability of 0.0003 S/m/month, and resolution of 0.00004 S/m at 24 samples per second. The conductivity cells have been replaced to newer style cells for deep ocean measurements. Pre-cruise sensor calibrations were performed at SBE, Inc. S/N 042435, 12 May 2016 S/N 041088, 12 May 2016 The value of conductivity at salinity of 35, temperature of 15 °C (IPTS-68) and pressure of 0 dbar is 4.2914 S/m. iv. Oxygen (SBE 43) The SBE 43 oxygen sensor uses a Clark polarographic element to provide in-situ measurements at depths up to 7000 m. The range for dissolved oxygen is 120 % of surface saturation in all natural waters, nominal accuracy is 2 % of saturation, and typical stability is 2 % per 1000 hours. Pre-cruise sensor calibration was performed at SBE, Inc. S/N 432471, 10 May 2016 v. Deep Ocean Standards Thermometer Deep Ocean Standards Thermometer (SBE 35) is an accurate, ocean-range temperature sensor that can be standardized against Triple Point of Water and Gallium Melt Point cells and is also capable of measuring temperature in the ocean to depths of 6800 m. The SBE 35 was used to calibrate the SBE 3 temperature sensors in situ (Uchida et al., 2007). Pre-cruise sensor linearization was performed at SBE, Inc. S/N 0045, 27 September 2002 Then the SBE 35 is certified by measurements in thermodynamic fixed- point cells of the TPW (0.01 °C) and GaMP (29.7646 °C). The slow time drift of the SBE 35 is adjusted by periodic recertification corrections. Pre-cruise sensor calibration was performed at SBE, Inc. Since 2014, fixed-point cells traceable to NIST temperature standards is directly used in the manufacturer’s calibration of the SBE 35 (Uchida et al., 2015). Since 2016, pre-cruise sensor calibration was performed at RCGC/JAMSTEC by using fixed- point cells traceable to NMIJ temperature standards. S/N 0045, 30 June 2016 (slope and offset correction) Slope = 1.000023 Offset = –0.001053 The time required per sample = 1.1 × NCYCLES + 2.7 seconds. The 1.1 seconds is total time per an acquisition cycle. NCYCLES is the number of acquisition cycles per sample and was set to 4. The 2.7 seconds is required for converting the measured values to temperature and storing average in EEPROM. Fig. 4.7.1: Time drifts (temperature offsets relative to the first calibration) of six reference thermometers (SBE 35) based on laboratory calibrations in fixed-point cells. Results performed at JAMSTEC are shown in red marks. vi. Altimeter Benthos PSA-916T Sonar Altimeter (Teledyne Benthos, Inc.) determines the distance of the target from the unit by generating a narrow beam acoustic pulse and measuring the travel time for the pulse to bounce back from the target surface. It is rated for operation in water depths up to 10000 m. The PSA-916T uses the nominal speed of sound of 1500 m/s. vii. Oxygen optode (RINKO) RINKO (JFE Alec Co., Ltd.) is based on the ability of selected substances to act as dynamic fluorescence quenchers. RINKO model III is designed to use with a CTD system which accept an auxiliary analog sensor, and is designed to operate down to 7000 m. Data from the RINKO can be corrected for the time-dependent, pressure-induced effect by means of the same method as that developed for the SBE 43 (Edwards et al., 2010). The calibration coefficients, H1 (amplitude of hysteresis correction), H2 (curvature function for hysteresis), and H3 (time constant for hysteresis) were determined empirically as follows. H1 = 0.0055 (for S/N 0024) H2 = 5000 dbar H3 = 2000 seconds Outputs from RINKO are the raw phase shift data. The RINKO can be calibrated by the modified Stern-Volmer equation slightly modified from a method by Uchida et al. (2010): O2 ((mol/l) = [(V0 / V)E – 1] / Ksv where V is voltage, V0 is voltage in the absence of oxygen, Ksv is Stern- Volmer constant. The coefficient E corrects nonlinearity of the Stern- Volmer equation. The V0 and the Ksv are assumed to be functions of temperature as follows. Ksv = C0 + C1 × T + C2 × T2 V0 = 1 + C3 × T V = C4 + C5 × Vb where T is CTD temperature (°C) and Vb is raw output (volts). V0 and V are normalized by the output in the absence of oxygen at 0°C. The oxygen concentration is calculated using accurate temperature data from the CTD temperature sensor instead of temperature data from the RINKO. The pressure-compensated oxygen concentration O2c can be calculated as follows. O2c = O2 (1 + Cpp / 1000) where p is CTD pressure (dbar) and Cp is the compensation coefficient. Since the sensing foil of the optode is permeable only to gas and not to water, the optode oxygen must be corrected for salinity. The salinity- compensated oxygen can be calculated by multiplying the factor of the effect of salt on the oxygen solubility (Garcia and Gordon, 1992). Pre-cruise sensor calibrations were performed at RCGC/JAMSTEC. S/N 0024, 10 May 2015 viii. Fluorometer The Seapoint Chlorophyll Fluorometer (Seapoint Sensors, Inc., Kingston, New Hampshire, USA) provides in-situ measurements of chlorophyll-a at depths up to 6000 m. The instrument uses modulated blue LED lamps and a blue excitation filter to excite chlorophyll-a. The fluorescent light emitted by the chlorophyll-a passes through a red emission filter and is detected by a silicon photodiode. The low level signal is then processed using synchronous demodulation circuitry, which generates an output voltage proportional to chlorophyll-a concentration. ix. Transmissometer The C-Star Transmissometer (WET Labs, Inc., Philomath, Oregon, USA) measures light transmittance at a single wavelength (650 nm) over a known path (25 cm). In general, losses of light propagating through water can be attributed to two primary causes: scattering and absorption. By projecting a collimated beam of light through the water and placing a focused receiver at a known distance away, one can quantify these losses. The ratio of light gathered by the receiver to the amount originating at the source is known as the beam transmittance. Suspended particles, phytoplankton, bacteria and dissolved organic matter contribute to the losses sensed by the instrument. Thus, the instrument provides information both for an indication of the total concentrations of matter in the water as well as for a value of the water clarity. Light transmission Tr (in %) and beam attenuation coefficient cp are calculated from the sensor output (V in volt) as follows. Tr = (c0 + c1 V) × 100 cp = – (1 / 0.25) ln(Tr / 100) Pre-cruise sensor calibration was performed at WET Labs. S/N CST-1726DR, 26 May 2015 x. Turbidity meter The Seapoint turbidity meter (Seapoint Sensors, Inc., Kingston, New Hampshire, USA) detects light scattered by particles suspended in water at depths up to 6000 m. The sensor generates an output voltage proportional to turbidity or suspended solids. The unique optical design confines the sensing volume to within 5 cm of the sensor. xi. PAR Photosynthetically Active Radiation (PAR) sensors (Satlantic, LP, Halifax, Nova Scotia, Canada) provide highly accurate measurements of PAR (400 – 700 nm) for a wide range of aquatic and terrestrial applications. The ideal spectral response for a PAR sensor is one that gives equal emphasis to all photons between 400 – 700 nm. Satlantic PAR sensors use a high quality filtered silicon photodiode to provide a near equal spectral response across the entire wavelength range of the measurement. Pre-cruise sensor calibration was performed at Satlantic, LP. S/N 1025, 6 July 2015 xii. CDOM The Environmental Characterization Optics (ECO) miniature fluorometer (WET Labs, Inc., Philomath, Oregon, USA) allows the user to measure relative Colored Dissolved Organic Matter (CDOM) concentrations by directly measuring the amount of fluorescence emission in a sample volume of water. The CDOM fluorometer uses an UV LED to provide the excitation source. An interference filter is used to reject the small amount of out- of-band light emitted by the LED. The light from the source enters the water volume at an angle of approximately 55-60 degrees with respect to the end face of the unit. Fluoresced light is received by a detector positioned where the acceptance angle forms a 140-degree intersection with the source beam. An interference filter is used to discriminate against the scattered excitation light. CDOM (Quinine Dihydrate Equivalent) concentration expressed in ppb can be derived using the equation as follows. CDOM = Scale Factor * (Output – Dark Counts) Pre-cruise sensor calibration was performed at WET Labs. S/N FLCDRTD-2014, 1 September 2015 Dark Counts: 0.025 V Scale Factor: 106 ppb/V (5) Data collection and processing i. Data collection CTD system was powered on at least 20 minutes in advance of the data acquisition to stabilize the pressure sensor and was powered off at least two minutes after the operation in order to acquire pressure data on the ship’s deck. The package was lowered into the water from the starboard side and held 10 m beneath the surface in order to activate the pump. After the pump was activated, the package was lifted to the surface and lowered at a rate of 1.0 m/s to 200 m (or 300 m when significant wave height was high) then the package was stopped to operate the heave compensator of the crane. The package was lowered again at a rate of 1.2 m/s to the bottom. For the up cast, the package was lifted at a rate of 1.1 m/s except for bottle firing stops. As a rule, the bottle was fired after waiting from the stop for more than 20 seconds and the package was stayed at least 5 seconds for measurement of the SBE 35 at each bottle firing stops. For depths where vertical gradient of water properties were expected to be large (from surface to thermocline), the bottle was exceptionally fired after waiting from the stop for 60 seconds to enhance exchanging the water between inside and outside of the bottle. At 200 m (or 300 m) from the surface, the package was stopped to stop the heave compensator of the crane. Water samples were collected using a 36-bottle SBE 32 Carousel Water Sampler with 12-litre Niskin- X bottles. Before a cast taken water for CFCs, the bottle frame and Niskin-X bottles were wiped with acetone. Data acquisition software SEASAVE-Win32, version 7.23.2 ii. Data collection problems (a) Miss trip, miss fire, and remarkable leak Miss trip, miss fire and remarkable leak occurred during the cruise were listed below. Miss trip Miss fire Leak none none 007_1 #20 end closure: O-ring of the end closure replaced 010_1 #21 end closure: O-ring of the end closure replaced 022_1 #22 end closure: O-ring of the end closure checked 024_1 #4 end closure: O-ring of the end closure checked (b) Slight leaks Slight leaks were observed from the root of stopcocks during drawing of the samples at station leg3_011_1 (#2, #4, #5, #7, #11, #12), leg3_015_1 (#25, #26, #27, #29), leg3_016_1 (#25, #27), leg3_018_1 (#3), and leg3_026_1 (#36). The bottle flags for those bottles were set to 2 since the bottle data (salinity and oxygen) were normal and there was no leak for those bottles at the leak check before the drawing of the samples. (c) Noise in down cast data Transmissometer data were noisy at station leg2_006_1 (504~506, 519~521, 820~826, 833~838, 939~947, 968~970, 1063~1067, 1255~1259 dbar), leg2_007_1 (117~118, 1022~1025 dbar), leg2_12B_1 (736~741, 1035~1037 dbar), leg2_11B_1 (131~133 dbar), leg3_009_1 (1071-1076 dbar), leg3_015_1 (821~826 dbar), leg3_016_1 (1497~1541, 1574~1578 dbar), leg3_021_1 (400~527 dbar), leg3_023_1 (992~998 dbar), leg3_024_1 (2248~2253 dbar) and leg3_025_1 (64~65, 473~475 dbar), and the data were removed and linearly interpolated. iii. Data processing SEASOFT consists of modular menu driven routines for acquisition, display, processing, and archiving of oceanographic data acquired with SBE equipment. Raw data are acquired from instruments and are stored as unmodified data. The conversion module DATCNV uses instrument configuration and calibration coefficients to create a converted engineering unit data file that is operated on by all SEASOFT post processing modules. The following are the SEASOFT and original software data processing module sequence and specifications used in the reduction of CTD data in this cruise. Data processing software SBEDataProcessing-Win32, version 7.23.2 DATCNV converted the raw data to engineering unit data. DATCNV also extracted bottle information where scans were marked with the bottle confirm bit during acquisition. The duration was set to 4.4 seconds, and the offset was set to 0.0 second. The hysteresis correction for the SBE 43 data (voltage) was applied for both profile and bottle information data. RINKOCOR (original module, version 1.0) corrected the time-dependent, pressure-induced effect (hysteresis) of the RINKO for both profile data. RINKOCORROS (original module, version 1.0) corrected the time- dependent, pressure-induced effect (hysteresis) of the RINKO for bottle information data by using the hysteresis-corrected profile data. BOTTLESUM created a summary of the bottle data. The data were averaged over 4.4 seconds. ALIGNCTD converted the time-sequence of sensor outputs into the pressure sequence to ensure that all calculations were made using measurements from the same parcel of water. For a SBE 9plus CTD with the ducted temperature and conductivity sensors and a 3000-rpm pump, the typical net advance of the conductivity relative to the temperature is 0.073 seconds. So, the SBE 11plus deck unit was set to advance the primary and the secondary conductivity for 1.73 scans (1.75/24 = 0.073 seconds). Oxygen data are also systematically delayed with respect to depth mainly because of the long time constant of the oxygen sensor and of an additional delay from the transit time of water in the pumped plumbing line. This delay was compensated by 5 seconds advancing the SBE 43 oxygen sensor output (voltage) relative to the temperature data. Delay of the RINKO data was also compensated by 1 second advancing sensor output (voltage) relative to the temperature data. Delay of the transmissometer data was also compensated by 2 seconds advancing sensor output (voltage) relative to the temperature data. WILDEDIT marked extreme outliers in the data files. The first pass of WILDEDIT obtained an accurate estimate of the true standard deviation of the data. The data were read in blocks of 1000 scans. Data greater than 10 standard deviations were flagged. The second pass computed a standard deviation over the same 1000 scans excluding the flagged values. Values greater than 20 standard deviations were marked bad. This process was applied to pressure, temperature, conductivity, and SBE 43 output. CELLTM used a recursive filter to remove conductivity cell thermal mass effects from the measured conductivity. Typical values used were thermal anomaly amplitude alpha = 0.03 and the time constant 1/beta = 7.0. FILTER performed a low pass filter on pressure with a time constant of 0.15 seconds. In order to produce zero phase lag (no time shift) the filter runs forward first then backwards. WFILTER performed as a median filter to remove spikes in fluorometer, turbidity meter, transmissometer, and CDOM data. A median value was determined by 49 scans of the window. For CDOM data, an additional box- car filter with a window of 361 scans was applied to remove noise. SECTIONU (original module, version 1.1) selected a time span of data based on scan number in order to reduce a file size. The minimum number was set to be the start time when the CTD package was beneath the sea- surface after activation of the pump. The maximum number was set to be the end time when the depth of the package was 1 dbar below the surface. The minimum and maximum numbers were automatically calculated in the module. LOOPEDIT marked scans where the CTD was moving less than the minimum velocity of 0.0 m/s (traveling backwards due to ship roll). DESPIKE (original module, version 1.0) removed spikes of the data. A median and mean absolute deviation was calculated in 1-dbar pressure bins for both down- and up-cast, excluding the flagged values. Values greater than 4 mean absolute deviations from the median were marked bad for each bin. This process was performed 2 times for temperature, conductivity, SBE 43, and RINKO output. DERIVE was used to compute oxygen (SBE 43). BINAVG averaged the data into 1-dbar pressure bins. The center value of the first bin was set equal to the bin size. The bin minimum and maximum values are the center value plus and minus half the bin size. Scans with pressures greater than the minimum and less than or equal to the maximum were averaged. Scans were interpolated so that a data record exist every dbar. BOTTOMCUT (original module, version 0.1) deleted the deepest pressure bin when the averaged scan number of the deepest bin was smaller than the average scan number of the bin just above. DERIVE was re-used to compute salinity, potential temperature, and density. SPLIT was used to split data into the down cast and the up cast. Remaining spikes in the CTD data were manually eliminated from the 1- dbar-averaged data. The data gaps resulting from the elimination were linearly interpolated with a quality flag of 6. (6) Post-cruise calibration i. Pressure The CTD pressure sensor offset in the period of the cruise was estimated from the pressure readings on the ship deck. For best results the Paroscientific sensor was powered on for at least 20 minutes before the operation. In order to get the calibration data for the pre- and post-cast pressure sensor drift, the CTD deck pressure was averaged over first and last one minute, respectively. Then the atmospheric pressure deviation from a standard atmospheric pressure (14.7 psi) was subtracted from the CTD deck pressure to check the pressure sensor time drift. The atmospheric pressure was measured at the captain deck (20 m high from the base line) and sub-sampled one-minute interval as a meteorological data. Time series of the CTD deck pressure is shown in Figs. 4.7.2 and 4.7.3. The CTD pressure sensor offset was estimated from the deck pressure. Mean of the pre- and the post-casts data over the whole period gave an estimation of the pressure sensor offset (0.66 dbar) from the pre-cruise calibration. The post-cruise correction of the pressure data was carried out by subtracting 0.66 dbar from the pressure data. Figs. 4.7.2 and 4.7.3 show the pressure data after the post-cruise correction. Fig. 4.7.2: Time series of the CTD deck pressure for leg 2. Atmospheric pressure deviation (magenta dots) from a standard atmospheric pressure was subtracted from the CTD deck pressure. Blue and green dots indicate pre- and post-cast deck pressures, respectively. Red dots indicate averages of the pre- and the post-cast deck pressures. Fig. 4.7.3: Same as Fig. 4.7.2, but for leg 3. ii. Temperature The CTD temperature sensors (SBE 3) were calibrated with the SBE 35 under the assumption that discrepancies between SBE 3 and SBE 35 data were due to pressure sensitivity, the viscous heating effect, and time drift of the SBE 3, according to a method by Uchida et al. (2007). Post-cruise sensor calibration for the SBE 35 will be performed at JAMSTEC in 2017 The CTD temperature was preliminary calibrated as Calibrated temperature = T – (c0 × P + c1 × t + c2 ) where T is CTD temperature in °C, P is pressure in dbar, t is time in days from pre-cruise calibration date of the CTD temperature and c0, c1, and c2 are calibration coefficients. The coefficients were determined using the data for the depths deeper than 1950 dbar. The coefficient c1 was set to zero for this cruise. The primary temperature data were basically used for the post-cruise calibration. The secondary temperature sensor was also calibrated and used instead of the primary temperature data when the data quality of the primary temperature data was bad. The calibration coefficients are listed in Table 4.7.1. The results of the post-cruise calibration for the CTD temperature are summarized in Table 4.7.2 and shown in Figs. 4.7.4 and 4.7.5. Table 4.7.1: Calibration coefficients for the CTD temperature sensors. Serial number c0(°C/dbar) c1(°C/day) c2(°C) ————————————— ———————————— —————————— ——————— 031525 –1.713992e–8 0.0 0.00029 Table 4.7.2: Difference between the CTD temperature and the SBE 35 after the post-cruise calibration. Mean and standard deviation (Sdev) are calculated for the data below and above 1950 dbar. Number of data used is also shown. Serial Pressure ≥ 1950 dbar Pressure < 1950 dbar number ———————————————————— ———————————————————— —————— Number Mean Sdev Number Mean Sdev (mK) (mK) (mK) (mK) —————— ———— ———— —————— ———— ———— 031525 326 0.0 0.2 616 –0.3 2.7 Fig. 4.7.4: Difference between the CTD temperature (primary) and the SBE 35 for leg 2. Blue and red dots indicate before and after the post-cruise calibration using the SBE 35 data, respectively. Lower two panels show histogram of the difference after the calibration. Fig. 4.7.5: Same as Fig. 4.7.4, but for leg 3. iii. Salinity The discrepancy between the CTD conductivity and the conductivity calculated from the bottle salinity data with the CTD temperature and pressure data is considered to be a function of conductivity, pressure and time. The CTD conductivity was calibrated as Calibrated conductivity = C – (c0 × C + c1 × P + c2 × C × P + c3 × P2 + c4 × P2 × C + c5 × P2 × C2 + c6) where C is CTD conductivity in S/m, P is pressure in dbar, and c0, c1, c2, c3, c4, c5 and c6 are calibration coefficients. The best fit sets of coefficients were determined by a least square technique to minimize the deviation from the conductivity calculated from the bottle salinity data. The primary conductivity data created by the software module ROSSUM were used after the post- cruise calibration for the temperature data. The calibration coefficients are listed in Table 4.7.3. The results of the post-cruise calibration for the CTD salinity are summarized in Table 4.7.4 and shown in Figs 4.7.6 and 4.7.7. Table 4.7.3: Calibration coefficients for the CTD conductivity sensors. Coefficient S/N 042435 ——————————— ————————————————— c0 7.2645896049e–6 c1 2.9691992467e–7 c2 –7.2958281688e–8 c3 1.9466613572e–10 c4 –1.6842918454e–10 c5 3.3411307753e–11 c6 –9.7770147557e–5 Table 4.7.4: Difference between the CTD salinity and the bottle salinity after the post-cruise calibration. Mean and standard deviation (Sdev) (in 10–3) are calculated for the data below and above 950 dbar. Number of data used is also shown. Serial Pressure ≥ 950 dbar Pressure < 950 dbar number ——————————————————— ——————————————————— —————— Number Mean Sdev Number Mean Sdev —————— ———— ———— —————— ———— ———— 042435 465 –0.1 0.6 390 0.1 3.1 Fig. 4.7.6: Difference between the CTD salinity (primary) and the bottle salinity for leg 2. Blue and red dots indicate before and after the post-cruise calibration, respectively. Lower two panels show histogram of the difference after the calibration. Fig. 4.7.7: Same as Fig. 4.7.6, but for leg 3. iv. Oxygen The RINKO oxygen optode (S/N 0024) was calibrated and used as the CTD oxygen data, since the RINKO has a fast time response. The pressure- hysteresis corrected RINKO data was calibrated by the modified Stern- Volmer equation, basically according to a method by Uchida et al. (2010) with slight modification: [O2] (µmol/l) = [(V0 / V)1.5 – 1] / Ksv and Ksv = C0 + C1 × T + C2 × T2 V0 = 1 + C3 × T V = C4 + C5 × Vb + C6 × t + C7 × t × Vb where Vb is the RINKO output (voltage), V0 is voltage in the absence of oxygen, T is temperature in °C, and t is working time (days) integrated from the first CTD cast. Time drift of the RINKO output was corrected. The calibration coefficients were determined by minimizing the sum of absolute deviation with a weight from the bottle oxygen data. The revised quasi-Newton method (DMINF1) was used to determine the sets. The post-cruise calibrated temperature and salinity data were used for the calibration. The calibration coefficients are listed in Table 4.7.5. The results of the post-cruise calibration for the RINKO oxygen are summarized in Table 4.7.6 and shown in Figs. 4.7.8 and 4.7.9. Table 4.7.5: Calibration coefficients for the RINKO oxygen sensors. Coefficient S/N 0024 ——————————— ————————————————————— c0 5.942125838095365e–3 c1 2.112922682529651e–4 c2 2.453149432631086e–6 c3 –2.858906729587995e–3 c4 –3.724762205027561e–2 c5 0.3277293704143511 c6 6.221125143791855e–4 c7 –5.158472610105331e–4 Cp 0.014 Table 4.7.6: Difference between the RINKO oxygen and the bottle oxygen after the post-cruise calibration. Mean and standard deviation (Sdev) are calculated for the data below and above 950 dbar. Number of data used is also shown. Serial Pressure ≥ 950 dbar Pressure < 950 dbar number ——————————————————— ——————————————————— —————— Number Mean Sdev Number Mean Sdev [mol/kg] [mol/kg] —————— ———— ———— —————— ————— ———— 0024 465 0.00 0.27 391 –0.10 0.88 Fig. 4.7.8: Difference between the CTD oxygen and the bottle oxygen for leg 2. Blue and red dots indicate before and after the post- cruise calibration, respectively. Lower two panels show histogram of the difference after the calibration. Fig. 4.7.9: Same as Fig. 4.7.8, but for leg 3. v. Fluorometer The CTD fluorometer (FLUOR in µg/L) was calibrated by comparing with the bottle sampled chlorophyll-a as FLUORc = c0 + c1 × FLUOR where c0 and c1 are calibration coefficients. The CTD fluorometer data is slightly noisy so that the up cast profile data which was averaged over one decibar agree with the bottle sampled data better than the discrete CTD fluorometer data obtained at bottle-firing stop. Therefore, the CTD fluorometer data at water sampling depths extracted from the up cast profile data were compared with the bottle sampled chlorophyll-a data. The bottle sampled data obtained at dark condition [PAR (Photosynthetically Available Radiation) < 50 3 nmol kg-1) were expected to be observed in the Indian Ocean. A commonly-encountered distribution in the upper ocean with a CH4 peak within the pycnocline (e.g., Ward et al. 1987; Owens et al. 1991; Watanabe et al. 1995; Yoshida et al. 2011). Karl and Tilbrook (1994) suggested the suboxic conditions would further aid the development of microenvironments within particles in which CH4 could be produced. The organic particles are accumulated in the pycnocline, and CH4 is produced in the micro reducing environment by methanogenic bacteria. Moreover, in situ microbial CH4 production in the guts of zooplankton can be expected (e.g., Owens et al. 1991; de Angelis and Lee 1994; Oudot et al. 2002; Sasakawa et al. 2008). Watanabe et al. (1995) pointed out that the diffusive flux of CH4 from subsurface maxima to air-sea interface is sufficient to account for its emission flux to the atmosphere. In the mixed layer above its boundary, the CH4 is formed and discharged to the atmosphere in part, in the below its boundary, CH4 diffused to the bottom vertically. By using concentration and isotopic composition of CH4 and hydrographic parameters for vertical water samples, it is possible to clarify its dynamics such as production and/or consumption in the water column. References Alldredge AA, Cohen Y (1987) Can microscale chemical patches persist in the sea? Microelectrode study of marine snow, fecal pellets. Science, 235:689-691 Alonso-Sáez L, Galand PE, Casamayor EO, Pedrós-Alió C, Bertilsson S (2010) High bicarbonate assimilation in the dark by Arctic bacteria. ISME J, 174:1581–90 Anantharaman K, Breier JA, Sheik CS, Dick GJ (2013) Evidence for hydrogen oxidation and metabolic plasticity in widespread deep-sea sulfur- oxidizing bacteria. Proceedings of the National Academy of Sciences, 110:330–335 Bange, HW, Bartell UH, Rapsomanikis S, Andreae MO (1994) Methane in the Baltic and the North seas and a reassessment of the marine emissions of methane. Global Biogeochemical Cycles, 8:465–480 Cicerone RJ, Oremland RS (1988) Biogeochemical aspects of atmospheric methane, Global Biogeochemical Cycles, 2:299–327 de Angelis MA, Lee C (1994) Methane production during zooplankton grazing on marine phytoplankton. Limnology and Oceanography, 39:1298- 1308 Dore JE, Popp BN, Karl DM, Sansone FJ (1998) A large source of atmospheric nitrous oxide from subtropical North Pacific surface water. Nature, 396:63-66 Francis CA, Beman JM, Kuypers MM (2007) New processes and players in the nitrogen cycle: the microbial ecology of anaerobic and archaeal ammonia oxidation. ISME J 1: 19–27 Granger J, Sigman DM (2009) Removal of nitrite with sulfamic acid for nitrate N and O isotope analysis with the denitrifier method. Rapid Communications in Mass Spectrometry, 23:3753-3762 Herndl GJ, Reinthaler T (2013) Microbial control of the dark end of the biological pump. Nature Geoscience, 6:718–724 IPCC Working group I (2013): Climate change 2013: The physical science basis. IPCC The 5th Assessment report, http://www.ipcc.ch/report/ar5/wg1/. Karl DM, Tilbrook BD (1994) Production and transport of methane in oceanic particulate organic matter. Nature, 368:732–734 Katz ME, Pak DK, Dickkens GR, Miller KG (1999) The source and fate of massive carbon input during the latest Paleocene thermal maximum. Science, 286:1531–1533 Knowles R, Lean DRS, Chan YK (1981) Nitrous oxide concentrations in lakes: variations with depth and time. Limnology and Oceanography, 26:855-866 Lelieveld J, Crutzen PJ, Dentener FJ (1998) Changing concentration, lifetime and climate forcing of atmospheric methane. Tellus Series B, 50:128–150 Maribeb CG, Laura F (2004) N2O cycling at the core of the oxygen minimum zone off northern Chile. Marine Ecology Progress Series, 280:1-11 Oudot C, Jean-Baptiste P, Fourre E, Mormiche Guevel C, Ternon JF-, Corre PL (2002) Transatlantic equatorial distribution of nitrous oxide and methane. Deep-Sea Research Part I, 49:1175–1193 Owens NJP, Law CS, Mantoura RFC, Burkill PH, Llewellyn CA(1991) Methane flux to the atmosphere from the Arabian Sea. Nature, 354:293–296 Rysgaard S, Risgaard-Petersen N, Nielsen LP, Revsbech NP (1993) Nitrification and denitrification in lake and estuarine sediments measured by the 15N dilution technique and isotope pairing. Applied and Environmental Microbiology, 59:2093-2098 Sasakawa M, Tsunogai U, Kameyama S, Nakagawa F, Nojiri Y, Tsuda A (2008) Carbon isotopic characterization for the origin of excess methane in subsurface seawater. Journal of Geophysical Research, 113:C03012, doi: 10.1029/2007JC004217 Santoro AE, Buchwald C, McIlvin MR, Casciotti KL (2011) Isotopic signature of N2O produced by marine ammonia-oxidizing Archaea. Science, 333:1282-1285 Sigman DM, Casciotti KL, Andreani M, Barford C, Galanter M, Boehlke JK (2001) A bacterial method for the nitrogen isotopic analysis of nitrate in seawater and freshwater. Analytical Chemistry, 73:4145- 4153 Stieglmeier M, Mooshammer M, Kitzler B, Wanek W, Zechmeister-Boltenstern S, Richter A, Schleper C (2014) Aerobic nitrous oxide production through N-nitrosating hybrid formation in ammonia-oxidizing archaea. ISME J, 8:1135-1146 Swan BK, Martinez-Garcia M, Preston CM, Sczyrba A, Woyke T, Lamy, D, Reinthaler T, Poulton NJ, Masland ED, Gomez ML, Sieracki ME, DeLong EF, Herndl GJ, Stepanauskas R (2011) Potential for chemolithoauto- trophy among ubiquitous bacteria lineages in the dark ocean. Science, 333:1296-1300 Svensson JM (1998) Emission of N2O, nitrification and denitrification in a eutrophic lake sediment bioturbated by Chironomus plumosus. Aquatic Microbial Ecology, 14:289-299 Tilbrook BD, Karl DM (1995) Methane sources, distributions and sinks from California coastal waters to the oligotrophic North Pacific gyre. Marine Chemistry, 49:51–64 Tsunogai U, Ishibashi J, Wakita H, Gamo T (1998) Methane-rich plumes in the Suruga Trough (Japan) and their carbon isotopic characterization. Earth and Planetary Science Letters, 160:97-105 Tsunogai U, Yoshida N, Ishibashi J, Gamo T (2000) Carbon isotopic distribution of methane in deep-sea hydrothermal plume, Myojin Knoll Caldera, Izu-Bonin arc: Implications for microbial methane oxidation in the oceans and applications to heat flux estimation. Geochimca et Cosmochimca Acta, 64:2439-2452 Ueda S, Ogura N, Yoshinari T (1993) Accumulation of nitrous oxide in aerobic ground water. Water Research, 27:1787-1792 Ward BB, Kilpatrick KA, Novelli PC, Scranton MI (1987) Methane oxidation and methane fluxes in the ocean surface layer and deep anoxic waters. Nature, 327:226–229 Watanabe S, Higashitani N, Tsurushima N, Tsunogai S (1995) Methane in the western North Pacific. Journal of Oceanography, 51:39–60 Yamagishi H, Westley MB, Popp BN, Toyoda S, Yoshida N, Watanabe S, Koba K, Yamanaka Y (2007) Role of nitrification and denitrification on the nitrous oxide cycle in the eastern tropical North Pacific and Gulf of California. J. Geophys. Res. Biogeosciences, doi:10.1029/2006JG000227 Yoshida N, Toyoda S (2000) Constraining the atmospheric N2O budget from intramolecular site preference in N2O isotopomers. Nature, 405:330- 334 Yoshida O, Inoue HY, Watanabe S, Noriki S, Wakatsuchi M (2004) Methane in the western part of the Sea of Okhotsk in 1998-2000. Journal of Geophysical Research, doi:10.1029/2003JC001910 Yoshida O, Inoue HY, Watanabe S, Suzuki K, Noriki S (2011) Dissolved methane distribution in the South Pacific and the Pacific Ocean in austral summer. Journal of Geophysical. Research, doi:10.1029/2009JC006089 Yoshikawa C, Abe H, Aita MN, Breider F, Kuzunuki K, Ogawa NO, Suga H, Ohkouchi N, Danielache SO, Wakita M, Honda MC, Toyoda S, Yoshida N (2016) Insights into the production processes of nitrous oxide in the western north Pacific by using a marine ecosystem isotopomer model. Journal of Oceanography, 72, 491–508 4.14 Vertical Profiles of Microbial Abundance, Activity and Diversity (1) Personnel Taichi Yokokawa (JAMSTEC) Michinari Sunamura (The University of Tokyo) Takuro Nunoura (JAMSTEC) (2) Introduction Prokaryotes (Bacteria and Archaea) play a major role in marine biogeochemical fluxes. Biogeochemical transformation rates and functional diversity of microbes are representative major topics in marine microbial ecology. However, the link between prokaryotes properties and biogeochemistry in the meso- and bathypelagic layers has not been explained systematically despite of the recent studies that highlight the role of microbes in the cycling of organic and inorganic matter. (Herndl and Reinthaler 2013; Yokokawa et al. 2013; Nunoura et al. 2015). Moreover, microbial diversity and biogeography in meso- and bathypelagic ocean and its relationship with upper layers and deep-water circulation have also not been well studied. The objectives of this study, which analyze the water columns from sea surface to just above the bottom of Southern Ocean, were 1) to determine the abundance of microbes; 2) to study the heterotrophic production of prokaryotes; 3) to assess the community composition of prokaryotes; 4) to know microbial diversity through water columns along the latitudinal transect. (3) Methods Microbial abundance Samples for microbial abundances (prokaryotes, eukaryotes and viruses) were collected in every routine cast and depth. Samples were fixed with glutaraldehyde (final concentration 1%) and/or mixed with Glycerol-EDTA, and frozen at -80°C. The abundance and relative size of microbes and viruses will be measured by a flow cytometry in both The University of Tokyo (Sunamura) and JAMSTEC (Yokokawa) after nucleic acid staining with SYBR-Green I. For the correction of flow cytometry data and morphological analysis of microbial cells, microbial cells in seawater were filtered and collected on polycarbonate membrane after formalin fixation. The filter samples were frozen at -80°C. The samples will be observed by fluorescent microscope at The University of Tokyo (Sunamura). Samples for fluorescent microscopy is collected at stn.1, 10 and 23. Microbial activity measurements Heterotrophic microbial production and microbial respiration were determined based on 3H-leucine incorporation rate and CTC-formazan reduction rate. 3H-leucine incorporation rate was determined as a proxy for heterotrophic or mixotrophic prokaryotic production. Triplicate subsamples (1.5 mL) dispensed into screw-capped centrifuge tubes amended with 10 nmol L-1 (final concentration) of [3H]-leucine (NET1166, PerkinElmer) and incubated at in situ temperature (± 2°C) in the dark. One trichloroacetic acid (TCA) killed blank was prepared for each sample. Incubation periods were 1 hour and 24 hours for the upper (0 – 250 m) and deeper (300 – bottom) water layers, respectively. After the incubation, proteins were TCA (final conc. 5%) extracted twice by centrifugation (15000 rpm, 10 min, Kubota 3615-sigma), followed by the extraction with ice-cold 80% ethanol. The samples will be radioassayed with a liquid scintillation counter using Ultima-GOLD (Packard) as scintillation cocktail. Quenching is corrected by external standard channel ratio. The disintegrations per minute (DPM) of the TCA-killed blank is subtracted from the average DPM of the samples, and the resulting DPM is converted into leucine incorporation rates. Tetrazolium salts are reduced by electron transport chain and produce formazan dye. Respiration microbial cell numbers and fluorescent intensities were determined based on the fluorescent CTC formazan. A 760nl of seawater was added in a 1.5ml protein low bind tube with a CTC tetrazolium salts (final conc. 5mM), Phenazine methoxy sulfate (final conc. 25sM), KCN (final conc. 1mM), Gly-TE. The tubes were incubated at in situ temperature (± 2°C) in the dark. Duplicate 150Gl of the incubated sample was subsampled into 96 well plate and frozen at -80°C to stop incubation at the incubation period of 2h, 8h, and 24h. Densities and fluorescent intensity of total microbial cells and CTC formazan produced cells will be measured by a flow cytometer (Attune / CytoFlex) after nucleic stain by SYBR Green I. Samples for leucine incorporation activity measurements and CTC reduction rates measurements were taken at stations 1, 4, 10, 13, 18, 21, 22 and 23 in the routine casts. Microbial diversity Microbial cells in water samples were filtrated on cellulose acetate filter (0.2µm) and stored at -80˚C. Environmental DNA or RNA will be extracted from the filtrated cells and used for 16S/18S rRNA gene tag sequencing using MiSeq, quantitative PCR for genes for 16S rRNA, and/or metatranscriptomics. Moreover, selected water samples were mixed with glycerol-EDTA and stored at -80˚C for single cell genomic analyses. Samples for microbial diversity were taken at stations 1, 4, 10, 13, 18, 21, 22 and 23 in the routine casts. References Herndl GJ, Reinthaler T (2013) Microbial control of the dark end of the biological pump. Nature geoscience, 6:718-724 Nunoura T, Takaki Y, Hirai M, Shimamura S, Makabe A, Koide O, Kikuchi T, Miyazaki J, Koba K, Yoshida N, Sunamura M, Takai K (2015) Hadal biosphere: Insight into the microbial ecosystem in the deepest ocean on Earth. Proceedings of the Natioanl Academy of Sciences 112:1230- 1236 Yokokawa T, Yang Y, Motegi C, Nagata T (2013) Large-scale geographical variation in prokaryotic abundance and production in meso- and bathypelagic zones of the central Pacific and Southern Ocean. Limnology and Oceanography, 58:61-73 4.15 Chlorophyll a (1) Personnel Kosei Sasaoka (JAMSTEC) (Leg 3) Takuhei Shiozaki (JAMSTEC) (Leg 2) Hironori Sato (MWJ) (Leg 1) Masanori Enoki (MWJ) (Leg 3) Misato Kuwahara (MWJ) (Leg 3) Haruka Tamada (MWJ) (Leg 3) Ei Hatakeyama (MWJ) (Leg 3) (2) Objectives Chlorophyll a is one of the most convenient indicators of phytoplankton stock, and has been used extensively for the estimation of phytoplankton abundance in various aquatic environments. In this study, we investigated horizontal and vertical distribution of phytoplankton around the Chilean coast (Leg 2) and along the P17E section (Leg 3) in the Southern Ocean. The chlorophyll a data is also utilized for calibration of fluorometers, which were installed in the surface water monitoring and CTD profiler system. (3) Instrument and Method Seawater samples were collected in 280 mL (Leg 2) and 500 mL (Leg 3) brown Nalgene bottles without head-space, and samples from the surface (0 m) were collected using a bucket. The whole samples were gently filtrated by low vacuum pressure (<0.02 MPa) through Whatman GF/F filter (diameter 25 mm) in the dark room. Whole volume of each sampling bottle was precisely measured in advance. After filtration, phytoplankton pigments were immediately extracted in 7 ml of N,N-dimethylformamide (DMF), and samples were stored at –20°C under the dark condition to extract chlorophyll a more than 24 hours. Chlorophyll a concentrations were measured by the Turner fluorometer (10-AU-005, TURNER DESIGNS), which was previously calibrated against a pure chlorophyll a (Sigma-Aldrich Co., LLC) (Figure 4.15.1). To estimate the chlorophyll a concentrations, we applied to the fluorometric “Non-acidification method” (Welschmeyer, 1994). (4) Results Vertical profiles of chlorophyll a concentrations around the Chilean coast (Leg 2) and along the P17E section (Leg 3) during the cruise are shown in Figure 4.15.2 and Figure 4.15.3, respectively. Cross section of chlorophyll a concentrations along the P17E line (Leg 3) is shown in Figure 4.15.4. To estimate the measurement precision, 34-pairs of replicate samples were obtained from hydrographic casts (Leg 3). All pairs of the replicate samples were collected in 500 ml bottles. Although the absolute values of the difference between 34-pairs replicate samples were 0-0.07 wg/L, those standard deviations were approximately 0.013. (5) Reference Welschmeyer, N. A. (1994): Fluorometric analysis of chlorophyll a in the presence of chlorophyll b and pheopigments. Limnor. Oceanogr., 39, 1985-1992. Figure 4.15.1: Relationships between pure chlorophyll a concentrations and fluorescence light intensity ((a) Leg 2, (b) Leg 1, 3, 4) Figure 4.15.2: Vertical profiles of chlorophyll a concentrations around the Chilean coast (Leg 2) obtained from hydrographic casts. Figure 4.15.3: Vertical profiles of chlorophyll a concentrations along the P17E section (Leg 3) obtained from hydrographic casts. Figure 4.15.4: Cross section of chlorophyll a concentrations along the P17E-line (Leg 3) obtained from hydrographic casts. 4.16 Nitrogen Fixation (1) Personnel Takuhei Shiozaki (JAMSTEC)-PI (2) Objectives Biological nitrogen fixation by specialized prokaryotic microorgan- isms (diazotrophs) converts dinitrogen gas into ammonia, and is a major source of reactive nitrogen in the ocean. Knowing the distribution and magnitude of oceanic nitrogen fixation, and what controls the biogeography of diazotrophs, is therefore essential for understanding the marine nitrogen cycle. Nitrogen fixation has historically been mainly measured for in the tropical and subtropical oligotrophic ocean regions where diazotrophs were expected to occur under the warm oligotrophic condition. However, recent studies show that nitrogen fixation also occurs in colder and/or nutrient-rich waters such as Arctic Ocean, temperate coastal water, river plumes, coastal upwelling regions, and nutrient-rich aphotic waters. Since such environments have only rarely been surveyed for nitrogen fixation in the past, the global nitrogen inputs by diazotrophs could potentially be much higher than previously thought. Here I examined nitrogen fixation from the surface to the bottom in the temperate Chilean coastal region. (3) Instruments and methods Water samples from the subsurface were collected in Niskin-X bottles, and samples from the surface (0 m) were collected using a bucket. Nitrogen fixation was determined by the 15N2 gas bubble method (Montoya et al., 1996, Appl. Environ. Microbiol. 62, 986-993), combined with a primary production assay using the 15N-13C dual inlet technique. Seawater samples were transferred into acid-cleaned 1–4.5 L polycarbonate bottles. 13C-labeled sodium bicarbonate (99 atom% 13C; Cambridge Isotope Laboratories, Inc., Andover, MA, USA) was added to the bottles at a final tracer concentration of 200 µmol L-1 before sealing it with a thermoplastic elastomer cap. Then, using a gas-tight syringe, 1–5 ml of 15N2 gas (99.8 atom% 15N; Shoko) was added to each bottle. The samples collected from the surface and 25 m were incubated in an on-deck incubator cooling by surface seawater and the samples from the aphotic zone were incubated in a thermostatic incubator under dark condition. The incubations were terminated by gentle vacuum filtration of the seawater samples through a precombusted GF/F filter after 24 h. Samples collected for estimating the initial 15N and 13C enrichment of particulate organic matter were filtered immediately at the beginning of the incubation. The filters were kept frozen (-20 °C) for on-shore analysis. (4) Data archives These data obtained in this cruise will be submitted to the Data Management Group of JAMSTEC when ready. 4.17 Absorption coefficients of particulate matter and colored dissolved organic matter (CDOM) (1) Personnel Kosei Sasaoka (JAMSTEC) (Leg 3) (2) Objectives Absorption coefficients of particulate matter (phytoplankton and non- phytoplankton particles, defined as ‘detritus’) and colored dissolved organic matter (CDOM) play an important role in determining the optical properties of seawater. In particular, light absorption by phytoplankton is a fundamental process of photosynthesis, and their chlorophyll a (Chl- a) specific coefficient, a*ph, can be essential factors for bio-optical models to estimate primary productivities. Absorption coefficients of CDOM are also important parameters to validate and develop the bio- optical algorithms for ocean color sensors, because the absorbance spectrum of CDOM overlaps that of Chl-a. The global colored detrital and dissolved materials (CDOM) distribution appears regulated by a coupling of biological, photochemical, and physical oceanographic processes all acting on a local scale, and greater than 50% of blue light absorption is controlled by CDOM (Siegel et al., 2002). Additionally, some investigators have reported that CDOM emerges as a unique tracer for diagnosing changes in biogeochemistry and the overturning circulation, similar to dissolved oxygen (e.g., Nelson et al., 2010). The objectives of this study are to understand the North-South variability of light absorption by phytoplankton and CDOM along the P17E section in the Southern Ocean. (3) Methods Seawater samples for absorption coefficient of total particulate matter (ap(λ)) were performed using Niskin bottles and a bucket above 100m depth at 7 stations along the P17E section (Fig.4.17-1, Table 4.17-1). Samples were collected in 3000ml dark bottles and filtered (500 - 3000 ml) through 25-mm What-man GF/F glass-fiber filters under a gentle vacuum (< 0.013 MPa) on board in the dark room. After filtration, the optical density of total particulate matter on filter (ODfp(λ)) between 350 and 750 nm at a rate of 1.0 nm was immediately measured by an UV-VIS recording spectrophotometer (UV-2400, Shimadzu Co.), and absorption coefficient was determined from the OD according to the quantitative filter technique (QFT) (Mitchell, 1990). A blank filter with filtered seawater was used as reference. All spectra were normalized to 0.0 at 750nm to minimize difference between sample and reference filter. To determine the optical density of non-pigment detrital particles (ODfd(λ)), the filters were then soaked in methanol for a few hours and rinsed with filtered seawater to extract and remove the pigments (Kishino et al., 1985), and its absorption coefficient was measured again by UV- 2400. These measured optical densities on filters (ODfp(λ) and ODfd(λ)) were converted to optical densities in suspensions (ODsp(λ) and ODsd(λ)) using the pathlength amplification factor of Cleveland and Weidemann (1993) as follows: ODsp(λ) = 0.378 ODfp(λ) + 0.523 ODfp(λ)2 and ODsd(λ) = 0.378 ODfd(λ) + 0.523 ODfd(λ)2. The absorption coefficient of total particles (ap(λ) (m-1)) and non- pigment detrital particles (ad(λ) (m-1)) are computed from the corrected optical densities (ODs(λ)): ap(λ) = 2.303 × ODsp(λ)/L (L = V/S), and ad(λ) = 2.303 × ODsd(λ)/L (L = V/S), Where S is the clearance area of the filter (m2) and V is the volume filtered (m3). Absorption coefficient of phytoplankton (aph(λ)) was obtained by subtracting ad(λ) from ap(λ) as follows: aph(λ) = ap(λ) − ad(λ). Finally, we calculated chl-a normalized specific absorption spectra (a*ph) to divide aph by chl-a concentrations obtained from same hydrographic casts. Seawater samples for absorption coefficient of CDOM (ay(λ)) were collected in 250ml bottles using Niskin bottles and a bucket from surface to bottom (Fig. 4.17-1, Table 4.17-1). CDOM samples were filtered using 0.2 µm Nuclepore polycarbonate filters on board. Optical densities of the CDOM (ODy(λ)) in this filtered seawater were recorded against UV-2600 in the range from 300 to 800 nm using 10-cm pathlength glass cells. Milli-Q water was used as a base line. A blank (Milli-Q water versus Milli-Q water) was subtracted from each wavelength of the spectrum. The absorption coefficient of CDOM (ay(λ) (m-1)) was calculated from measured optical densities (ODy(λ)) as follows: ay(λ) = 2.303 × ODy(λ/ L (L is the cuvette path-length (m)). (4) Preliminary results Chl-a normalized specific absorption spectra (a*ph) were shown in Fig.4.17-2. Vertical profiles and cross section of CDOM (as absorption coefficient at 325 nm, unit = m-1) along the P17E section were shown in Fig. 4.17-3 and Fig.4.17-4. (5) References Cleveland, J.S. and Weidemann, A.D., 1993, Quantifying absorption by aquatic particles: a multiple scattering correction for glass fiber filters, Limnology and Oceanography, 38, 1321-1327. Kishino, M., Takahashi, M., Okami, N. and Ichimura, S., 1985, Estimation of the spectral absorption coefficients of phytoplankton in the sea, Bulletin of Marine Science, 37, 634-642. Mitchell, B.G., 1990, Algorithms for determining the absorption coefficient of aquatic particulates using the quantitative filter technique (QFT), Ocean Optics X, SPIE 1302, 137-148. Nelson, N. B., D. A. Siegel, C. A. Carlson, and C. M. Swan, 2010, Tracing global biogeochemical cycles and meridional overturning circulation using chromophoric dissolved organic matter, Geophys. Res. Lett., 37, L03610, doi:10.1029/2009GL042325. Siegel, D.A., Maritorena, S., Nelson, N.B., Hansell, D.A., Lorenzi- Kayser, M., 2002, Global distribution and dynamics of colored dissolved and detrital organic materials. J. Geophys. Res., 107, C12, 3228, doi:10.1029/2001JC000965. Fig. 4.17-1: Location of 7-sampling stations for absorption coefficients of phytoplankton and CDOM along the P17E section in the Southern Ocean during MR16-09 (Leg 3). Table 4.17-1: List of sampling stations for absorption coefficients of phytoplankton (Ap) and CDOM during MR16-09 (Leg 3). Stn Date (UTC) Time(UTC) Latitude Longitude Sampling type Cast No. Sampling depth (db) Particle absorbance CDOM absorbance 1 02/16/2017 7:39 67.00 S 125.98 W CTD + Bucket 2 0, Chlmax(20), 10, 50, 100 3797, Chlmax(20), 3000, 1000, 800, 600, 400, 200, 100, 50, 10, 0 4 02/17/2017 5:28 65.02 S 125.96 W CTD + Bucket 1 0, Chlmax(30), 10, 50, 100 4953, Chlmax(30), 3000, 1000, 800, 600, 400, 200, 100, 50, 10, 0 8 02/18/2017 22:29 62.34 S 126.11 W CTD + Bucket 1 0, Chlmax(65), 10, 50, 100 5143, Chlmax(65), 3080, 1070, 830, 630, 430, 200, 100, 50, 10, 0 12 02/20/2017 0:36 60.01 S 125.98 W CTD + Bucket 1 0, Chlmax(80), 10, 50, 100 4683, Chlmax(80), 2930, 970, 770, 570, 370, 200, 100, 50, 10, 0 16 02/20/2017 20:58 58.01 S 126.00 W CTD + Bucket 1 0, Chlmax(75), 10, 50, 100 4321, Chlmax(75), 2930, 970, 770, 570, 370, 200, 100, 50, 10, 0 21 02/21/2017 19:47 55.50 S 125.98 W CTD + Bucket 1 0, Chlmax(65), 10, 50, 100 3576, Chlmax(65), 2930, 970, 770, 570, 370, 200, 100, 50, 10, 0 24 02/22/2017 11:19 54.01 S 125.98 W CTD + Bucket 1 0, Chlmax(30), 10, 50, 100 3541, Chlmax(30), 2930, 970, 770, 570, 370, 200, 100, 50, 10, 0 Fig.4.17-2: Chlorophyll-specific phytoplankton absorption coefficient spectra (a*ph(λ)) at 400-750 nm. All spectra were normalized to 0.0 at 750nm. Fig.4.17-3: Vertical profiles of CDOM (as absorption coefficient at 325 nm, unit = m-1) at 7-stations along the P17E section. Fig.4.17-4: Contours showing distribution of CDOM (as absorption coefficient at 325 nm, unit = m-1) along the P17E section. 4.18 Calcium (1) Personnel Etsuro Ono (JAMSTEC) (2) Objectives Calcium is one of the major dissolved components in the sea water. Many corals and marine organisms consume calcium to produce calcium carbonate (CaCO3) as their shells and skeletons. According to the recent IPCC report, ocean acidification is progressing, because about 30% of the anthropogenic carbon dioxide has been absorbed into the ocean. Ocean acidification is characterized by an increase of H+ (i.e., a decrease of pH) and a concurrent decrease of carbonate ion concentration (CO32–). The decrease of CO32– promotes dissolution of CaCO3, which is unfavorable to marine calcifying organisms. In this cruise, to evaluate dissolution and precipitation of calcium carbonate, we measured directly the concentration of calcium in the sea water in a subantarctic region of the Southern Pacific Ocean and the Antarctic Ocean. (3) Instruments The analysis system consisted of a modified Dissolved Oxygen Titrator (DOT-01: Kimoto Electronic Co. Ltd.) which had a band-pass filter centered at 620 nm, a xenon light source, a photodiode detectors, and Auto-Burette system with control unit (Kimoto Electronic Co. Ltd.). (4) Sampling and analytical methods The samples from niskin sampler were collected to 60ml of HDPE bottles from niskins. After sampling, the samples were stored at a cool and dark place for about 7days before measurement. The measurement method of calcium was based on a photometric method suggested by Culkin and Cox (1966). The reagents and the procedure of the measurement in this cruise were as follows: ・Reagents Titrant : 0.02 mol/l EGTA (Ethylene Glycol Tetraacetic Acid) Buffer : Mixture solution of 0.4 mol/l NH4Cl and 0.4 mol/l NH3 Indicator : 4mmol/l Zincon® solution Zinc source : Mixuture solution of 8mmol/l ZnSO4 and 8mmol/l EGTA ・Pretreatment of sea samples 10ml of seawater was transferred into a tall beaker by a volumetric pipet. A stirrer tip was put into the sample. 1ml of buffer solution was added to keep the solution at pH 9.5. 1ml of Zincon indicator was added which stained the sample red. 1ml of Zinc source was added which turned the sample blue. Mille-Q water was added such that the overall solution was approx. 80ml. (When measuring the acidic standard solution, the solution was neutralized by the solution of sodium hydroxide (NaOH) before buffer solution was added.) (5) Preparation of standard solution The in-house Ca-standard was prepared for determination of the concentration of EGTA titrant. The concentration of the standard solution was 10mmol/l, which was calculated by the gravimetric method. For preparation of the standard solution, pure CaCO3 produced by NMIJ (CRM 3013-a) was used as Ca-source. Pure CaCO3 was in advance dried in an oven at 110℃ for 2 hours and accurately weighed at 1.0009g, then 50ml of 0.5M HCl solution was added to CaCO3 until CaCO3 was dissolved completely and degas CO2 from the solution. After bubbles in the degassing solution calmed down, the solution was transferred to a 1000ml volumetric flask, with pure water added until 1000ml, and the weight of the whole solution was measured. The acidity of the standard solution was about pH=2.0. The density of the Ca-standard solution was necessary to calculate the concentration of the standard solution. The method is described in Section 4.11 (Density). (6) Calibration of EGTA titrant In this cruise, two standard solutions were measured for monitoring the concentration of titrant. One is the in-house Ca-standard and the other is 1000mg/ L Calcium Standard Solution produced by Wako Pure Chemical Industries, Ltd. Volume of the standard solution for the monitoring measurement was 10ml for the in-house Ca-standard and 4ml for the Wako standard, so that calcium level was close to that of the sea samples. Figure 4.18.1 shows the end point values (ml) of titration and their trends. The end point values tend to decrease. Also, the trend of the value in the in-house Ca-standard measurement is similar to that in the Wako standard. Thus, it’s assumed that the concentration of EGTA titrant was increasing during the sample measurements because of evaporation of solvent caused by the headspace in the bottle of titrant. The variation of the concentration was not negligible, because the magnitude of that was more than 0.1% c.v. Therefore, the calibration of EGTA titrant was carried out by fitting a linear function calculated from the in-house Ca- standard. Fig. 4.18.1: Plots of the end point of standard measurements. Fig. 4.18.2: Plots and calibration line for EGTA titrant. (7) Interference to titrations by magnesium A previous work (Culkin and Cox, 1966) points out that magnesium (Mg) and strontium (Sr) cause positive bias to the titrated volume of Ca because of their interference with the reaction between EGTA and Ca; the bias caused by Mg was 0.729% and by Sr was 0.388%. Also, in our preparation before the cruise, when Ca-standard with Mg source in same proportion as sea water was measured, it was suggested that the end point of that was increased by 0.745% as compared with the sample without Mg. This result agreed with the previous work. Although Mg interferes the titration of Ca in this titrating condition, no correction was given to the data submitted in this cruise. Table 4.18.1: Results of interference by Mg Average end point [ml] 2σ N —————————————————————— —————— — No Mg 5.1136 0.0076 9 Add Mg 5.1517 0.0046 9 Fig. 4.18.3: Comparison of the end point for Ca-standard added Mg and not containing Mg. (8) Performance The replicate samples were collected from 2 layers at each station to examine repeatability. The precision of replicate samples was estimated at 0.0052 mmol kg-1 (n=20 pairs). We used the SOP23 method to estimate the repeatability. There were no major troubles with the analysis during the cruise. Fig. 4.18.4: Vertical profiles of calcium. References F. Culkin, and R. A. Cox (1966) Sodium, potassium, magnesium, calcium and strontium in sea water. Deep-Sea Res., 13, 789-804. 4.19 Dissolved organic matter and the associated parameters (1) Personnel Masahito Shigemitsu (JAMSTEC): Principal investigator Taichi Yokokawa (JAMSTEC) Masahide Wakita (JAMSTEC) Akihiko Murata (JAMSTEC) (2) Objectives Dissolved organic matter (DOM) in the ocean can be affected by advection and mixing and DOM has relatively refractory fractions which resist biological degradation. Such characteristics of DOM play some important roles in the ocean biogeochemistry: 1) DOM contributes to the biological pump, which makes the dissolved organic carbon (DOC) in the ocean one of the major carbon reservoirs in the Earth, and 2) Dissolved organic nitrogen (DON) and dissolved organic phosphorus (DOP) can be carried away from the regions where those are produced, making DON and DOP the potential nutrients in the oligotrophic ocean. In this cruise, we aim to gain insights into the behavior of DOC in the Southern Ocean which is considered to be a key region for the oceanic carbon cycles, and clarify the spatial variations in ratio of DOC:DON:DOP to get some information about the importance of DON and DOP as potential nutrients. (3) Material and methods i. DOC and DON Seawater samples were obtained from Niskin bottles on a CTD-rosette system. Each sample taken in the upper 250 m was filtered using a pre- combusted (450℃ for 4 hours) Whatman 47-mm GF/F filter. The filtration was carried out by connecting a spigot of the Niskin bottle through silicone tube to an inline plastic filter holder. Filtrates were collected in acid-washed 60 mL High Density Polyethylene (HDPE) bottles in duplicates, and were immediately stored frozen until analysis. Other samples taken below 250 m were unfiltered and stored in the same way. In the analysis after this cruise, the frozen samples are thawed at room temperature, and acidified to pH < 2 with 50% HCl followed by being bubbled to remove dissolved inorganic carbon (DIC) from the samples. Then, the concentrations of DOC and total dissolved nitrogen (TDN) are measured with a total organic carbon analyzer equipped with a chemiluminescence detector unit (Shimadzu, Japan). Concentration of DON is calculated by subtracting the sum of dissolved inorganic nitrogen (nitrate, nitrite and ammonium) from the measured TDN. The measurement procedure of dissolved inorganic nitrogen is found somewhere in this cruise report. ii. Surface DOC, DON and DOP Sea-surface waters (5 m depth) were collected in the sea surface monitoring laboratory once a day along the cruise track except for the Chilean and New Zealand EEZs. The seawater samples were filtered in the similar way to the above. DOC and TDN concentrations for the samples are measured in the same way as stated above, and DON concentration is also calculated as stated above. Soluble reactive phosphorus (SRP) concentration is measured manually by the molymbdenum blue method (Parsons et al., 1984), and concentration of total dissolved phosphorus (TDP) is determined by the method after persulfate oxidation (Menzel and Corwin, 1965). DOP is calculated as difference between TDP and SRP. iii. Rates of DOC production and DIC fixation Seawater samples for measurements of rates of DOC production and DIC fixation were obtained at depths. The measurement procedure is basically based on the method of Teira et al. (2003). At each depth at each station, three samples of 30 ml were inoculated with 1480 kBq of NaH14CO3 followed by the incubations in an on-deck incubator. Incubation was stopped by adding 20% glutaraldehyde, and the seawater samples were filtered through 0.2µm cellulose filters. Filter samples are exposed to concentrated HCl fumes and filtrates are bubbled with N2 gas after addition of 50% HCl. Then, scintillation cocktail is added to filter and filtrate samples, and the radioactivity of them is measured by a liquid scintillation counter. Triplicate blank tests for 0.2µm-filtered seawater were carried out in the same way as the samples. (4) Data archives The data of each DOM and the associated parameters obtained in this cruise will be submitted to the Data Management Group of JAMSTEC, and will be open to the public via “Data Research System for Whole Cruise Information in JAMSTEC (DARWIN)” in JAMSTEC web site. (5) References Parsons, T.R., Y. Maita, C.M. Lalli (1984), A Manual for Chemical and Biological Methods for Seawater Analysis. Pergamon, Oxford. Menzel, D.W., and N. Corwin (1965), The measurement of total phosphorus in seawater based on the liberation of organically bound fractions by persulfate oxidation, Limnol. Oceanogr., 10, 280–282. Teira, E., M.J. Pazo, M. Quevedo, M.V. Fuentes, F.X. Niell, and E. Fernandez (2003), Rates of dissolved organic carbon production and bacterial activity in the eastern North Atlantic Subtropical Gyre during summer, Mar. Ecol. Prog. Ser., 249, 53-67. 4.20 Carbon isotopes March 3, 2017 (1) Personnel Yuichiro Kumamoto Japan Agency for Marine-Earth Science and Technology (2) Objective In order to investigate the water circulation and carbon cycle in the eastern Indian Ocean, seawaters for measurements of carbon-14 (radiocarbon) and carbon-13 (stable carbon) of total dissolved inorganic carbon (TDIC) were collected by the hydrocasts from surface to near bottom. (3) Sample collection The sampling stations and number of samples are summarized in Table 4.20.1. All samples for carbon isotope ratios (total 254 samples) were collected at 8 stations using 12-liter Niskin-X bottles. The seawater sample was siphoned into a 250 cm3 glass bottle with enough seawater to fill the glass bottle 2 times. Immediately after sampling, 10 cm3 of seawater was removed from the bottle and poisoned by 0.1 cm3 3l of saturated HgCl2 solution. Then the bottle was sealed by a glass stopper with Apiezon grease M and stored in a cool and dark space on board. (4) Sample preparation and measurements In our laboratory, dissolved inorganic carbon in the seawater samples will be stripped cryogenically and split into three aliquots: radiocarbon measurement (about 200 µmol), carbon-13 measurement (about 100 µmol), and archive (about 200 µmol). The extracted CO2 gas for radiocarbon will be then converted to graphite catalytically on iron powder with pure hydrogen gas. The carbon-13 of the extracted CO2 gas will be measured using Finnigan MAT253 mass spectrometer. The carbon-14 in the graphite sample will be measured by Accelerator Mass Spectrometry (AMS). Table 4.20.1: Sampling stations and number of samples for carbon isotope ratios. Number of Max. Stn Lat. (S) Long. (W) Sampling Number of replicate Pressure Date (UTC) samples samples (dbar) ——— ———————— ————————— —————————— ————————— ————————— ———————— 01 67-00.00 125-58.56 2017/02/16 28 2 3797 06 63-41.01 125-59.58 2017/02/17 33 2 5045 10 60-58.71 126-04.20 2017/02/19 31 2 4635 13 59-36.44 126-03.24 2017/02/20 31 2 4749 16 58-00.63 125-59.76 2017/02/20 30 2 4321 20 56-00.65 125-57.36 2017/02/21 29 2 4157 23 54-28.36 125-59.10 2017/02/22 27 2 3676 26 53-00.73 126-00.06 2017/02/22 29 2 4341 ———————————————————————————————————————————————————————————————————— Total 238 16 4.21 Stable Isotopes of Water February 28, 2017 (1) Personnel Hiroshi Uchida (JAMSTEC) Katsuro Katsumata (JAMSTEC) (2) Objectives The objective of this study is to collect stable isotopes of water to use as a tracer of ocean circulation. (3) Materials and methods The hydrogen (H) and oxygen (O) isotopic ratio of seawater are defined as follows: δD [‰] = 1000 {(D/H)sample/(D/H)VSMOW – 1} δ18O [‰] = 1000 {(18O/16O)sample/(18O/16O)VSMOW – 1} where D is deuterium and VSMOW is Vienna Standard Mean Ocean Water. The isotopic ratios of VSMOW water are defined as follows: (D/H)VSMOW = 155.76 ± 0.1 ppm (18O/16O)VSMOW = 2005.20 ± 0.43 ppm. The isotopic ratios will be measured in a laboratory in the Japan Agency for Marine-Earth Science and Technology, Yokosuka, Japan, after the cruise with a Cavity Ring-Down Spectroscopy (CRDS, L112-i, Picarro Inc., Santa Clare, CA, USA). The water samples were collected in 10-mL borosilicate glass bottles (Butyl rubber stopper with aluminum cap, Maruemu Co., Osaka, Japan). The collected samples are storing at room temperature. A total of 587 samples was collected including 34 pairs of replicate samples. 4.22 Beryllium Isotopes March 3, 2017 (1) Personnel Yuichiro Kumamoto Japan Agency for Marine-Earth Science and Technology (2) Objective 10Be (half-life 1.36 x 10^6 y) is produced in the atmosphere by cosmic rays. Its production rate is dependent on latitude, altitude and time, because the intensity of the cosmic rays is not homogeneous. The radionuclide is transported by aerosols, and moved from the stratosphere to the surface soil and surface ocean via the troposphere. Rates of production and precipitation of 10Be were calculated by Lal and Peters (1964), but their calculation has not been confirmed experimentally. The purpose of this study is to reveal a depth profile of 7Be and 10Be in the Antarctic Ocean. (3) Sample collection Total 18 of seawater sample (40L or 20L) for beryllium isotopes were collected at Station 1 (67.002°S/125.983°W, 16 Feb. 2017). The seawaters were sampled vertically using 12-liter Niskin-X bottles from the surface to the bottom of the water column. The seawater sample was collected into a 20-L plastic container and after two time washing. (4) Sample preparation and measurements To recover beryllium isotopes from large volume (40L or 20L) seawater samples, 2 mg of Be carrier, 2g of Fe carrier and 20ml of conc. HCl are added. After three hours or more later, 20ml of conc. NH4OH are added to the solution to co-precipitate Be(OH)2 and Fe(OH)3. Precipitates of Be(OH)2 and Fe(OH)3 are dissolved by conc. HCl, then concentrated and adjusted to 9M HCl solutions by adding conc. HCl for isopropyl ether extraction. Extraction procedure is repeated three times to remove Fe. The purification for Accelerator Mass Spectrometry (AMS) measurement uses a cation exchange column. For 9Be measurements, 250 ml of filtered seawater samples are separately stored in polypropylene bottles. 9Be is measured using a ICP- MS. 7Be and 10Be are measured using AMS at MALT, Univ. of Tokyo. 4.23 Lowered Acoustic Doppler Current Profiler (1) Personnel Shinya Kouketsu (JAMSTEC) (principal investigator) Hiroshi Uchida (JAMSTEC) Katsurou Katsumata (JAMSTEC) (2) Overview of the equipment An acoustic Doppler current profiler (ADCP) was integrated with the CTD/RMS package. The lowered ADCP (LADCP), Workhorse Monitor WHM300 (Teledyne RD Instruments, San Diego, California, USA), which has 4 downward facing transducers with 20-degree beam angles, rated to 6000 m. The LADCP makes direct current measurements at the depth of the CTD, thus providing a full profile of velocity. The LADCP was powered during the CTD casts by a 48 volts battery pack. The LADCP unit was set for recording internally prior to each cast. After each cast the internally stored observed data was uploaded to the computer on-board. By combining the measured velocity of the sea water and bottom with respect to the instrument, and shipboard navigation data during the CTD cast, the absolute velocity profile can be obtained (e.g. Visbeck, 2002). The instrument used in this cruise was as follows. Teledyne RD Instruments, WHM300 S/N 20754 (downward looking), S/N 18324 (upward looking) (3) Data collection In this cruise, data were collected with the following configuration. Bin size: 4.0 m Number of bins: 25 Pings per ensemble: 1 Ping interval: 1.0 sec Reference Visbeck, M. (2002): Deep velocity profiling using Lowered Acoustic Doppler Current Profilers: Bottom track and inverse solutions. J. Atmos. Oceanic Technol., 19, 794-807. 4.24 Micro Rider (1) Personnel Shinya Kouketsu (JAMSTEC) Hiroshi Uchida (JAMSTEC) Katsurou Katsumata (JAMSTEC) (2) Objective Microstructure observations to evaluate vertical mixing. (3) Instruments and method Micro structure observations were carried out by micro-Rider 6000 (MR6000; Rockland Scientific International Inc.), which is mounted CTD rosette and is powered from SBE 9plus. We mounted two FP07 thermistors to obtain the high-frequency changes in temperature. We sometimes replaced the probes during this cruise to compare sensitivities between the probes. The high-frequency pressure and acceleration profiles are also obtained by the sensors in MR6000. The low-frequency profiles of temperature are archived in the MR6000 from the cables connected with SBE-3 sensor on the CTD system. We download the profile data from the MR6000 a cast. After the cruise, we plan to examine the methods of the correction and measurement quality evaluation with the comparison among the micro temperature with CTD rosette, those with free fall instruments, and free fall micro shear structure observations. (4) Micro-Temperature measurement history * Sensor socket 1: T1320 * Sensor socket 2: T1337 (St. 1-2), T1338 (St. 3-4), T1339 (St. 5-13) and T1341 (St. 14-26) 4.25 Sound Velocity May 10, 2017 (1) Personnel Hiroshi Uchida (JAMSTEC) (Principal investigator) Rei Ito (MWJ) (Legs 2 and 3) Sonoka Tanihara (MWJ) (Leg 2) Kenichi Katayama (MWJ) (Leg 3) Shungo Oshitani (MWJ) (Leg 3) Rio Kobayashi (MWJ) (Leg 3) (2) Objectives The objective of this study is to estimate Absolute Salinity (also called “density salinity”) from sound velocity data with temperature and pressure data from CTD, and to evaluate an algorithm to estimate absolute salinity provided along with TEOS-10 (the International Thermodynamic Equation of Seawater 2010) (IOC et al., 2010). (3) Materials and methods Sound velocity profiles were measured at the CTD casts by using a velocimeter (MiniSVP, serial no. 49618, Valeport Ltd., Devon, United Kingdom). The sound velocity sensing elements are a ceramic transducer (signal sound pulse of 2.5 MHz frequency), a signal reflector, and spacer rods to control the sound path length (10 cm), providing a measurement at depths up to 6000 m. The velocimeter was attached to the CTD frame and level of the sound path of the velocimeter was same as that of the CTD temperature sensor, just next to the primary temperature sensor. Although temperature and pressure data were also measured by the velocimeter, only sound velocity data measured at a sampling rate of 8 Hz were combined with the CTD temperature and pressure data measured at a sampling rate of 24 Hz to estimate Absolute Salinity. The sound velocity data were obtained at all CTD casts in legs 2 and 3. The sound velocity data were roughly combined with the CTD data to match the time going into and coming out of the sea water, and the combined data were interpolated at a sub-sampling rate of 16 Hz. Time difference between the sound velocity data and the CTD data were more strictly adjusted to minimize spikes of salinity data back calculated from the sound velocity, pressure and temperature data as follows. Standard deviations of difference between the back calculated salinity data and their low-pass filtered data by a running mean with a window of 161 scans (10 seconds) were calculated for a segment from 20 to 70 dbar of the down cast by advancing the sound velocity data against the CTD data from –6 scans to +6 scans at one scan intervals, and the advanced scan to minimize the standard deviation was estimated. These calculations were repeated for a segment at 50 dbar intervals from 20 dbar to 570 dbar, and a median of the estimated advanced scans was calculated as the best estimate of the advanced scan. The estimated Absolute Salinity (Sv) were calibrated in situ referred to the Absolute Salinity measured by a density meter for water samples. The corrected Absolute Salinity were estimated as Corrected Absolute Salinity = (c0 + c1×Sv +c2×T + c3×P + c4×Sv2 + c5×P2 + c6×T2 + c7×Sv×P + c8×Sv×T) × (1 + c9×P) where T is CTD temperature in °C, P is pressure in dbar, and c0 ~ c8 are calibration coefficients. The best fit sets of coefficients were determined by a least square technique to minimize the deviation from the Absolute Salinity measured by the density meter, except for the coefficient c9 which was subjectively determined in advance. The post-cruise calibrated temperature and salinity data were used for the calibration. The calibration coefficients are listed in Table 4.25.1. The results of the post-cruise calibration for the Absolute Salinity estimated from the sound velocity data are summarized in Table 4.25.2 and shown in Fig. 4.25.1. Vertical profiles of the corrected Absolute Salinity were shown in Fig. 4.25.2. Table 4.25.1: Calibration coefficients for Absolute Salinity estimated from the sound velocity data. Coefficient S/N 49618 ——————————— ————————————————————— c0 26.70938514122043 c1 –0.5416586809715309 c2 –0.1354291356712744 c3 1.401399009550316e–3 c4 2.245731443302312e–2 c5 5.894712917405537e–8 c6 1.067486700100993e–3 c7 –9.109068401397720e–5 c8 3.551854573705933e–3 c9 5.17e–5 Table 4.25.2: Difference between the corrected Absolute Salinity estimated from the sound velocity data and the Absolute Salinity measured by the density meter after the post- cruise calibration. Mean and standard deviation (Sdev) are calculated for the data below and above 950 dbar. Number of data used is also shown. Serial number Pressure ≥ 950 dbar Pressure < 950 dbar —————— ————————————————————— ————————————————————— Number Mean Sdev Number Mean Sdev [g/kg] [g/kg] —————— ——————— —————— —————— —————— —————— —————— 49618 227 0.0000 0.0238 227 0.0000 0.0036 Fig. 4.25.1: Vertical distribution of differences between Absolute Salinity estimated from sound velocity data and Absolute Salinity estimated from the density meter for legs 2 and 3. Fig. 4.25.2: Vertical profiles of Absolute Salinity estimated from sound velocity data. Black lines indicate Reference-Composition Salinity derived from CTD salinity data. (4) Reference IOC, SCOR and IAPSO (2010): The international thermodynamic equation of seawater – 2010: Calculation and use of thermodynamic properties. Intergovernmental Oceanographic Commission, Manuals and Guides No. 56, United Nations Educational, Scientific and Cultural Organization (English), 196 pp. 4.26 pH, POC, and HPLC sampling for SOCCOM project (1) Personnel K. Katsumata (JAMSTEC) K. Sasaoka (JAMSTEC) E. Boss (University of Maine), A. Dickson (Scripps Institution of Oceanography) S. Becker (Scripps Institution of Oceanography) L. Talley (Scripps Institution of Oceanography) R. Key (Princeton University) (2) Objectives SOCCOM (Southern Ocean Carbon and Climate Observations and Modeling) is a project funded by NSF, NOAA, and NASA. The primary goal is to better understand the role of Southern Ocean in climate change and biogeochemistry with special emphasis on carbon flux and inventory. The main observational tool is a newly developed Argo-type float additionally equipped with biogeochemical sensors. The long term plan is to deploy approximately 200 floats in the Southern Ocean from 2014 to 2020. As a JAMSTEC contribution towards this project, we deployed five floats during the P17E reoccupation in the southeastern Pacific. It is essential that the float deployment be accompanied with high-quality bottle data for calibrating the float sensors. GO-SHIP cruises strives for state-of-the- art accuracy and precision and are consequently an ideal platform for this purpose. In this section, we describe the bottle sampling accompanying the float deployments. The float deployments are described in Section 5.2. (3) Stations and depths At five stations (2, 4, 8, 18, and 24) water samples were collected from Niskin bottles mounted in a Rosette sampler. Samples for pH were collected from all Niskins shallower than 2000 dbar, but not from the surface bucket sampling. Duplicate samplings were collected at two depths. Samples for HPLC and POC were collected from the Niskins near the chlorophyll maximum (when exists) or at a depth between the two bottles near the surface (usually 50 dbar and 100 dbar), when no obvious chlorophyll maximum was found. We monitored the fluorescence during CTD downcast to identify the chlorophyll maximum. Another set of samples was collected from the surface bucket sampling. Chlorophyll maximum sampling was duplicated. (4) pH The sampling method followed the instructions in Talley et al. (2017). Water samples were collected immediately after dissolved oxygen and CFCs. A Tygon tube designated solely for pH sampling was used to avoid possible contamination with other samples (DOC, in particular). After filling a bottle following a 20 second overflow, 16 mL of sampled sea water were removed by syringe and 120 µL of saturated mercuric chloride was added with an Eppendorf pipette. The bottles were then sealed and the contents mixed by inverting the bottle more than five times. The bottles were kept at about 5°C until 27th March 2017 when they were unloaded at Hachinohe port. The bottles were then air-freighted to Scripps Institution, San Diego for analysis. (5) HPLC and POC Samples were collected in brown Nalgene bottles using a silicone tube from Niskin bottles or a bucket. HPLC and POC were usually the last items to sample. Before collection, the Nalgene bottles and bucket were rinsed 3 times. After sampling, the sea water was immediately filtered in a dark room. One to three liters of sea water, depending on water clarity, were filtered and the volumes recorded. The filters were kept in a deep freezer at −80 °C. The samples were transferred to a dry shipper cooled with liquid nitrogen on 27th March 2017 at Hachinohe. They were subsequently air-freighted to Scripps Institution, San Diego for analysis. References Talley, L.D., S. Becker, R. Key, A. Dickson, E. Boss, C. Sakamoto, 2017, SOCCOM BGC floats shipboard calibration data requirement, version 8 January 2017, available online at https://soccom.princeton.edu/content/manuals 4.27 Chlorofluorocarbons and Sulfur hexafluoride Ken’ichi Sasaki (Mutsu Institute for Oceanography, JAMSTEC) Hironori Sato (Marine Works Japan Ltd.) Hiroshi Hoshino (Marine Works Japan Ltd.) Masahiro Orui (Marine Works Japan Ltd.) 1 Objectives Chlorofluorocarbons (CFCs) and sulfur hexafluoride (SF6) are man-made stable gases. These atmospheric gases can slightly dissolve in sea surface water by air-sea gas exchange and then are spread into the ocean interior. So dissolved these gases could be used as chemical tracers for the ocean circulation. We measured concentrations of three chemical species of CFCs, CFC-11 (CCl3F), CFC-12 (CCl2F2), and CFC-113 (C2Cl3F3), and SF6 in seawater on board, and made simultaneous analysis of dissolved nitrous oxide (N2O) for a certain number of seawater samples on the trial base. 2 Apparatus We use three measurement systems. One of them is CFCs analyzing system. Other two are SF6/CFCs simultaneous analyzing system. Trial analysis of N2O was made on latter systems. Both systems are based on purging and trapping gas chromatography. Table 4-27-1: Instruments SF6/CFCs (&N2O) simultaneous analyzing system ————————————————————————————————————————————— Gas Chromatograph: GC-14B (Shimadzu Ltd.) Detector 1: ECD-14 (Shimadzu Ltd.) Detector 2: ECD-14 (Shimadzu Ltd.) Analytical Column: Pre-column 1: Silica Plot capillary column [i.d.: 0.53 mm, length: 6 m, film thickness: 6 µm] Pre-column 2: Molesive 5A Plot capillary column [i.d.: 0.53 mm, length: 5 m, film thickness: 15 µm] Main column 1: Connected two capillary columns (Pola Bond-Q [i.d.: 0.53mm, length: 9 m, film thickness: 10µm] followed by Silica Plot [i.d.: 0.53mm, length: 18 m, film thickness: 6µm]) Main column 2: Connected two capillary columns (Molesive 5A Plot [i.d.: 0.53 mm, length: 3 m, film thickness: 15 µm] followed by Pola Bond-Q [i.d.: 0.53mm, length: 9 m, film thickness: 10µm]) Purging & trapping: Developed in JAMSTEC. Cold trap columns are 30 cm length stainless steel tubing packed the section of 5cm with 80/100 mesh Porapak Q and followed by the section of 5cm of 100/120 mesh Carboxen 1000. Outer diameters of the main and focus trap columns are 1/8” and 1/16”, respectively. CFCs analyzing system ————————————————————— Gas Chromatograph: GC-14B (Shimadzu Ltd.) Detector: ECD-14 (Shimadzu Ltd.) Analytical Column: Pre-column: Silica Plot capillary column [i.d.: 0.53mm, length: 6 m, film thickness: 6µm] Main column: Connected two capillary columns (Pola Bond-Q [i.d.: 0.53mm, length: 9 m, film thickness: 10µm] followed by Silica Plot [i.d.: 0.53mm, length: 18 m, film thickness: 6µm]) Purging & trapping: Developed in JAMSTEC. Cold trap columns are 1/16” SUS tubing packed the section of 5cm with 100/120 mesh Porapak T. 3 Procedures 3.1 Sampling Seawater sub-samples were collected from 12 liter Niskin bottles to 450 ml of glass bottles developed in JAMSTEC. The glass bottles were filled by CFC free gas (pure nitrogen gas) before sampling. Two times of the bottle volume of seawater sample were overflowed. The seawater samples were kept in a thermostatic water bath at 7ºC. The samples were taken to determination as soon as possible after sampling (usually within 12 hours). In order to confirm CFC/SF6 concentrations of standard gases and their stabilities and also to check saturation levels in sea surface water, mixing ratios in background air were periodically analyzed. Air samples were continuously led into laboratory by air pump. The end of 10 mm OD Dekaron tubing was put on a head of the compass deck and another end was connected onto the air pump in the laboratory. The tubing was relayed by a T-type union which had a small stop cock. Air sample was collected from the flowing air into a 200ml glass cylinder attached on the cock. 3.2 Analysis SF6/CFCs /N2O simultaneous analyzing system ——————————————————————————————————————————— Constant volume of sample water (200 ml) is taken into a sample loop. The sample is send into stripping chamber and dissolved SF6, CFCs and N2O are de-gassed by N2 gas purging for 8 minutes. The gas sample is dried by magnesium perchlorate desiccant and concentrated on a main trap column cooled down to -80 ºC. Stripping efficiencies are frequently confirmed by re-stripping of surface layer samples and more than 99 % of dissolved SF6 and CFCs and ~95 % of N2O are extracted on the first purge. Following purging & trapping, the main trap column is isolated and electrically heated to 180 ºC. After 1 minute, the desorbed gases are sent onto focus trap cooled down to -80 ºC for 30 seconds. Gaseous sample on the focus trap are desorbed by same manner of the main trap, and lead onto the pre-column 1 (PC 1). Sample gases are roughly separated on the PC 1. Eluting SF6, CFCs and N2O onto pre-column 2 (PC 2), PC1 is connected onto cleaning line and high boiling point compounds are flushed by counter flow of pure nitrogen gas. SF6 and CFCs are quickly eluted from PC 2 onto main-column 1 (MC 1) and N2O is retained on PC 2. Then PC 2 is connected back-flush carrier gas line and N2O is sent onto main- column 2 (MC 2). SF6 and CFCs are further separated on MC 1 and detected by ECD 1. N2O sent onto MC 2 is detected by ECD 2. CFCs analyzing system ————————————————————— Constant volume of sample water (50 ml) is taken into a sample loop. The sample is send into stripping chamber and dissolved CFCs are de-gassed by N2 gas purging for 8 minutes. The gas sample is dried by magnesium perchlorate desiccant and concentrated on a trap column cooled down to -50 ºC. Stripping efficiencies are frequently confirmed by re-stripping of surface layer samples and more than 99.5 % of dissolved CFCs are extracted on the first purge. Following purging & trapping, the trap column is isolated and electrically heated to 140 ºC. The desorbed gases are lead into the pre-column. Sample gases are roughly separated in the pre-column. When CFC-113 eluted from pre-column onto main column, the pre-column is connected onto another line and flushed by counter flow of pure nitrogen gas. CFCs send on MC 1 are further separated and detected by ECD. Nitrogen gases used in these systems was filtered by gas purifier column packed with Molecular Sieve 13X (MS-13X). Table 4-27-2: Analytical conditions SF6/CFCs(/N2O) simultaneous analyses ———————————————————————————————————— Temperature Analytical Column: 95°C Detector (ECD): 300°C Trap column: -80°C (at adsorbing) & 170°C (at desorbing) Mass flow rate of nitrogen gas (99.99995%) Carrier gas 1: 10 ml/min Carrier gas 2: 10 ml/min Detector make-up gas 1: 27 ml/min Detector make-up gas 2: 27 ml/min Back flush gas: 10 ml/min Sample purge gas: 220 ml/min CFCs analyses ————————————— Temperature Analytical Column: 95ºC Detector (ECD): 240ºC Trap column: -50ºC (at adsorbing) & 140ºC (at desorbing) Mass flow rate of nitrogen gas (99.99995%) Carrier gas : 10 ml/min Detector make-up gas: 27 ml/min Back flush gas: 10 ml/min Sample purge gas: 130 ml/min Standard gas (Japan Fine Products co. Ltd.) Cylinder No. Base CFC-11 CFC-12 CFC113 SF6 N2O remarks gas ppt ppt ppt ppt ppm ———————————— ———— —————— —————— —————— ———— ———— ——————————————— CPB20785 N2 873 472 81.5 9.83 14.6 for SF6/CFC/N2O CPB21090 N2 891 472 82.0 9.77 15.0 for SF6/CFC/N2O CPB09873 N2 301 160 30.2 0.00 0.0 for CFC CPB16993 N2 300 161 29.8 0.00 0.0 Reference 4 Performance The analytical precisions were estimated from replicate sample analyses. The estimated preliminary precisions were ± 0.014 pmol/kg (n = 69), ± 0.007 pmol/kg (n = 69), ± 0.007 pmol/kg (n = 69), ± 0.018 fmol/kg (n = 42), and ± 0.8 nmol/kg (n = 13) for CFC-11, CFC-12, CFC-113, SF6, and N2O, respectively. There were some problems on N2O analysis. The peak area of N2O was significantly increase at standard gas analysis after seawater sample analysis compared with that at continuous analysis of standard gas. This increase was not due to carryover from previous seawater sample analysis because any nitrous oxide peak does not detected in blank analysis just after a seawater sample analysis. As a possibility, a slight moisture in the sample gas could influence the sensitivity of the detector during seawater sample analysis. Further investigations are necessary for this phenomenon. As a stopgap measure on this cruise, calibration curves for nitrous oxide were prepared as following procedure. Standard gas was introduced into the system (and concentrated on cold trap) in the usual gas analysis sequence and immediately the N2 gas flow path was switched to the sea water line containing the blank seawater. This method can analyze the standard gas under almost same condition as the seawater analysis. In order to take a priority in the accuracy of CFCs and SF6, this procedure was not applied to the frequent standard gas analysis for sensitivity correction during sea water sample analysis. So accurate sensitivity correction would be difficult for N2O analyses. A peak area of N2O always became unusually small at the first seawater analysis after the standard gas analysis by the usual gas analysis sequence. This also seems to be the same cause that could be a lack of moisture. In this case, N2O measurement was not reported (flag "5" was given) because the correction methods for such measurement has not been found at the present time. 5 Data archive All data will be submitted to Data Management Group (DMG) of JAMSTEC. 5 Floats, Drifters and Moorings 5.1 Argo floats (1) Personnel Shuhei Masuda (JAMSTEC/RCGC): Principal Investigator (not on board) Shigeki Hosoda (JAMSTEC/ RCGC): not on board Kanako Sato (JAMSTEC/ RCGC): not on board Mizue Hirano (JAMSTEC/ RCGC): not on board Shingo Oshitani (MWJ): Technical Staff (Operation Leader) (2) Objectives The purpose of this study is to clarify the mechanisms of climate and oceanic environment variability for understanding changes of earth system through estimations of heat and material transports, by sustainably monitoring in the global ocean. To get knowledge of those changes in the ocean, it is crucial to obtain well-quality controlled observational data. As the Southern Ocean is one of the area where the number of active Argo float is unsatisfied to the target spatial density, which had been defined by the International Argo program, oceanic change is not well- understood although the Southern Ocean is one of the key region for climate changes. Especially physical process of the oceanic change below 2000m depth and biogeochemical process associated with global carbon cycle etc. are not yet recognized because of less amount of long-term ocean observations. To obtain physical and biogeochemical data in the Southern Ocean, we launched three Argo floats for measurements of temperature and salinity above 2000m depth, one deep Argo (Deep NINJA) for measurements temperature and salinity above 4000m depth and one deep/biogeochemical Argo (DO-Deep APEX) for measurements temperature, salinity and dissolved oxygen above 6000m depth at station points where shipboard CTD cast was conducted. The continuously obtaining data form those floats will be opened as contribution of the Argo program, after conducting real-time quality control within 24 hours by Argo data assembly center and delayed mode quality controls within one year by JAMSTEC as Argo PI. Based on the Argo and deep/biogeochemical Argo data, we will investigate spatial and temporal variability of water mass such as Antarctic Intermediate Water and amount of carbon uptake and transport, adapting those data to data assimilation systems such as JAMSTEC’s 4D-VAR data synthesis system (ESTOC). Further, we will evaluate accuracy of CTD and DO sensors mounted on the floats in comparison with the high accuracy shipboard CTD data at the station points, which makes Argo and deep/biogeochemical Argo data quality improve and then largely contributes to the International Argo program. (3) Parameters Water temperature, salinity, pressure, and dissolved oxygen (4) Methods i. Profiling float deployment of Argo We launched one Navis float with SBE41 CTD sensor and two Arvor floats with SBE41 CTD sensor. The floats usually drift at a depth of 1000 dbar (parking depth), then dive to a depth of 2000 dbar (profiling depth) and rise up to the sea surface by changing its buoyancy every ten days. The floats measure temperature, salinity, and pressure when they rise to the sea surface. During staying at the sea surface within a few ten minutes ~ several hours, observed data are transmitted to the base station via telecommunication satellites in real-time. The specifications of floats and launching points are shown in Table 5.1.1. Table 5.1.1: Specification of Navis/Arvor floats and launching point Float Type Navis EBR Arvor (manufacturer) (Sea-Bird Electronics Inc.) (nke instrumentation) CTD sensor SBE41 (Sea-Bird Electro- SBE41 (Sea-Bird Electro nics Inc.) nics Inc.) Cycle 10 days 10 days Iridium Router-Based Unrestricted Argos system transmit Digital Internetworking type Connectivity Solutions (RUDICS) Target 2000 dbar 2000 dbar Profiling Pressure Target 1000 dbar 1000 dbar Parking Pressure Sampling 2 dbar 5~20 dbar interval (approximately 1000 levels) (approximately 115 levels) Mission control Available Not available after launching Launching point Float S/N WMOID Date and Time Location CTD St. of Launch(UTC) of Launch No. ———————————————— ——————— ——————————————— ———————————————— ——————— F0415 5905051 2017/2/20 22:52 58° 0.828' [S] P17E16 (NAVIS) 125° 59.688' [W] OIN 13JAP-ARL-78 7900692 2017/2/19 14:47 60° 57.888' [S] P17E10 (Arvor) 125° 59.772' [W] OIN 13JAP-ARL-79 5905052 2017/2/21 21:24 55° 30.69[S] (Arvor) 125° 57.09[W] P17E21 ii. Profiling float deployment for biogeochemical/deep Argo We also launched one deep/biogeochemical Argo float (DO-Deep APEX) and one deep Argo float (Deep NINJA). The Deep NINJA equipped with SBE41 for deep CTD sensor, and the DO-Deep APEX equipped with SBE61 CTD sensor and Optode4831 dissolved oxygen sensor. The floats measure using above sensors when they go up to the sea surface. During staying at the sea surface within a few ten minutes, observed data are transmitted as the same style as for the Argo floats shown in (4) i. Specifications and their launching points are shown in Table 5.1.2. Table 5.1.2: Specification of Deep NINJA/DO-Deep APEX and launching point Float Type Deep NINJA Deep APEX (manufacturer) (Tsurumi Seiki Co.,Ltd) (Teleedyne Webb Research) CTD sensor SBE41 for Deep SBE61 (Sea-Bird Electronics Inc.) (Sea-Bird Electronics Inc.) Dissolved N/A Optode4831 Oxygen Sensor (Aanderaa Data Instruments) Cycle 5 days 5 days Iridium Short Burst Data Service Router-Based Unrestricted Digital transmit type (SBD) Internetworking Connectivity Solutions (RUDICS) Target Parking 2000 dbar 2000 dbar Pressure Target Profil- 4000 dbar 6000 dbar ing Pressure Sampling 5 dbar 5 dbar interval (approximately 800 levels) (approximately 1200 levels) Mission control Available Available after launching Ice detection Included Included Launching point Float WMO ID Date and Time Location of CTD St. No. S/N of Launch(UTC) Launch ————— ——————— ———————————————— ———————————————— ——————————— 20 7900691 2017/02/19 14:41 60° 58.008' [S] P17E-10 125° 59.982' [W] 45 Not yet 2017/02/19 14:34 60° 58.140 [S] P17E-10 obtained 126° 0.258' [W] (5) Data archive With regard to NAVIS, Arvor and Deep NINJA, observed data are delivered to meteorological organizations, research institutes, and universities etc. via Global Data Assembly Center (GDAC: http://www.usgodae.org/argo/argo.html, http://www.coriolis.eu.org/) andGlobal Telecommunication System (GTS). Real-time and delayed mode quality controls are conducted within 24 hours and one year after receiving the data, respectively. Both data are provided from GDACs following procedure decided by the International Argo program. With regard to SBE61 on DO-Deep APEX, the data will not delivered via GDACs for a while because quality control method is not yet fixed in the Argo Data Management Team. Instead, we will provide the data from Argo JAMSTEC HP conducting quality checks. Fig. 5.1.1: First profiles of vertical temperature and salinity distribution from NAVIS (WMOID: 5905051), Arvor (WMOID: 7900692 and 5905052) and Deep NINJA (WMOID: 7900691 but only above 2000m depth). 5.2 SOCCOM biogeochemical floats (1) Personnel K. Katsumata (JAMSTEC), S. Riser, D. Swift (University of Washington), K. Johnson (Monterey Bay Aquarium Research Institute), E. Boss (U. Maine), L. Talley (Scripps Institution of Oceanography) (2) Objectives SOCCOM (Southern Ocean Carbon and Climate Observations and Modeling) is a project funded by NSF, NOAA, and NASA aiming at understanding the roles of Southern Ocean in climate change and biogeochemistry of the Earth system. Their main observational tool is a newly developed float with biogeochemical measurements. The project envisages deploying approximately 200 such floats within the Southern Ocean from 2014 to 2020. As a JAMSTEC contribution towards the project, we have deployed five floats during the P17E reoccupation. It is essential that the float deployment be accompanied with high-quality bottle data for calibrating the float sensors. GO-SHIP cruises, which strive for state-of-the-art accuracy and precision in CTD and chemistry analyses are a good platform for this purpose. In this section, we describe the float deployments. The accompanying bottle sampling is described in Section 4.26 of this report. (4) SOCCOM BGC float In addition to the usual temperature and salinity measurements, a SOCCOM biogeochemical Argo-type float carries sensors to measure acidity (pH), nutrient (nitrate), and oxygen. The APEX floats that were deployed in this cruise also carried a bio-optic sensor to measure ocean fluorescence and backscatter. Further references for the float specifications are available at SOCCOM (2017). (5) Deployments Five floats were deployed at five different CTD stations right after the CTD cast. After cleaning the FLBB and ISUS sensors with pre- moistened lens cleaning wipe and deionized water following Riser et al. (2017), the floats were deployed from the stern deck of R/V Mirai with a rope. The details of deployments are shown below. The year is 2017. Stn Latitude Longitude Depth Time (UT) Float Serial Num. ——— —————————— ——————————— —————— ———————————— ————————————————— 2 66-21.55°S 126- 1.47°W 4445 m 16 Feb 17:33 12371 4 65-1.00°S 125-56.51°W 4872 m 17 Feb 07:42 12379 8 62-20.59°S 126- 6.90°W 5055 m 19 Feb 00:43 12366 18 57-1.60°S 126- 0.12°W 4115 m 21 Feb 07:26 12386 24 54-0.00°S 125-58.42°W 3543 m 22 Feb 13:01 12542 References Riser, S., R. Rupan, D. Swift, K. Johnson, C. Sakamoto, L. Talley, 2017, SOCCOM BGC Floats: Deployment and Cleaning Procedures, version 8 January 2017, available online at https://soccom.princeton.edu/content/manuals SOCCOM, 2017, https://soccom.princeton.edu/content/float- specifications 5.3 CO2 buoys (1) Personnel Akihiko Murata (JAMSTEC) Kosei Sasaoka (JAMSTEC) Tomonori Watai (MWJ) Atsushi Ono (MWJ) Emi Deguchi (MWJ) Nagisa Fujiki (MWJ) (2) Objective It is said that the ocean takes up approx. 30% of CO2 emitted into the atmosphere by human activities such as fossil fuel burning, deforestation, cement production, etc. Thus, accurate estimation of CO2 uptake by the ocean is an important task in predicting global warming and related climate changes, because the ocean tends to moderate the warming by absorbing anthropogenic CO2 from the atmosphere. Calculation of air- sea fluxes of CO2 is one of straightforward methods to estimate the CO2 uptake. Data for surface seawater partial pressure of CO2 (pCO2) are necessary for the calculation. Surface seawater pCO2 data covering the world ocean have been collected by such an international activity as Surface Ocean Carbon Dioxide Atlas (SOCAT). However, in spite of the long-term effort over 40 years, a large data gap is still found in the Southern Hemisphere oceans, especially in the South Pacific. This is because the ocean is far away from pCO2 observations-leading countries, i.e., difficult to do observations by research vessels due to high cost, and because there scarcely exist regular lines of cargo ships, along which pCO2 observations have been conducted. Drifting buoys with pCO2 sensor are free from the limitation. Therefore, we intend to deploy drifting buoys in the South Pacific during the MR16-09 cruise. (3) Apparatus The drifting pCO2 buoy was constructed by NiGK Corporation. The specification of drifting CO2 buoy is as Table 5.3.1. Table 5.3.1: Specification of drifting CO2 buoy. Items Specification ——————————————— ——————————————————————————————————————— Size Diameter: 315 mm (max.), Height: 575 mm Weight 8.6 kg Pressure proof 5 m Positioning GPS Battery Primary lithium battery CO2 range 150 111000 ppm CO2 resolution < 1 ppm Accuracy < 1.5% (5) Results We injected 7 drifting CO2 buoys into the South Pacific, where a large data gap exists. We injected them during the cruise of R/V Mirai (legs 1 and 3 of MR16-09) (Figs. 5.3.1 and 5.3.2), and started data acquisition through a satellite communication system. In addition, we introduced a server in order to stock, control and analyze data from drifting CO2 buoys. Fig. 5.3.1: Positions (circles) of drifting CO2 buoys injected during the R/V Mirai cruise and the Fig. 5.3.2: Drifting CO2 buoys on the deck of the R/V Mirai (left), and appearance of injection in the MR16-09 cruise (right). DATA HISTORY • File Merge Carolina Berys Cruise_Report_MR16-09_20170725.pdf (download) #64290 Date: 2018-04-25 Current Status: merged • File Merge Jerry Kappa 49NZ20170208_do.pdf (download) #38917 Date: 2018-04-25 Current Status: dataset • File Submission Jerry Kappa 49NZ20170208_do.pdf (download) #38917 Date: 2018-04-25 Current Status: dataset Notes The pdf version of the P17E_2017 cruise report is merged. It contains all the PI-provided data reports, CCHDO summary pages and CCHDO data processing notes. • File Merge CCHSIO 49NZ20170208_ct1.zip (download) #4454c Date: 2018-02-15 Current Status: merged • Update CTD exchange and netcdf files CCHSIO Date: 2018-02-15 Data Type: CTD Action: Website Update Note: 2017 49NZ20170208 processing - CTD/merge - CTDPRS,CTDTMP,CTDSAL,CTDSVLSAL,CTDOXY,CTDFLUOR,CTDXMISS,CTDXMISSCP,CTDTURB, CTDPAR,CTDCDOMF 2018-02-15 CCHSIO Submission filename submitted for date id -------------------- ------------- ---------- ----- 49NZ20170208_ct1.zip K.Katsumata 2017-04-04 12688 Changes ------- 49NZ20170208_ct1.zip - added units comments - added cruise information as commented header - changed file name to match CCHDO format - SECT_ID: changed header SECT to SECT_ID - XMISSCP: XMISSCP_FLAG_W not submitted, CCHDO copied XMISS_FLAG_W to XMISSCP_FLAG_W - CTDCDOMF: Changed parameter name from CDOM to CTDCDOMF - CTDCDOMF_FLAG_W: Changed parameter name from CDOM_FLAG_W to CTDCDOMF_FLAG_W - CTDFLUOR: Changed parameter name from FLUOR to CTDFLUOR - CTDFLUOR_FLAG_W: Changed parameter name from FLUOR_FLAG_W to CTDFLUOR_FLAG_W - CTDPAR: Changed parameter name from PAR to CTDPAR - CTDPAR_FLAG_W: Changed parameter name from PAR_FLAG_W to CTDPAR_FLAG_W - CTDSVLSAL: Changed parameter name from SVLSAL to CTDSVLSAL - CTDSVLSAL_FLAG_W: Changed parameter name from SVLSAL_FLAG_W to CTDSVLSAL_FLAG_W - CTDTURB: Changed parameter name from TURB to CTDTURB - CTDTURB_FLAG_W: Changed parameter name from TURB_FLAG_W to CTDTURB_FLAG_W - CTDXMISS: Changed parameter name from XMISS to CTDXMISS - CTDXMISSCP: Changed parameter name from XMISSCP to CTDXMISSCP - CTDXMISS_FLAG_W: Changed parameter name from XMISS_FLAG_W to CTDXMISS_FLAG_W - CTDCDOMF: Changed units from MG/CUM to MG/M^3 - CTDFLUOR: Changed units from MG/CUM to MG/M^3 - CTDXMISSCP_FLAG_W not submitted, copied CTDXMISS_FLAG_W to CTDXMISSCP_FLAG_W - CTDTURB, CTDCDOMF, CTDXMISSCP, and SVLSAL are not defined in Exchange format. - PAR unit UE/SQM/S is not a defined unit for PAR in Exchange format - CTDSVLSAL_FLAG_W: changed all flags from 1 to 9 because all CTDSVLSAL values are -999 Conversion ---------- file converted from software ----------------------- -------------------- ----------------------- 49NZ20170208_nc_ctd.zip 49NZ20170208_ct1.zip hydro 0.8.2-48-g594e1cb Updated Files Manifest ---------------------- file stamp ----------------------- -------------- 49NZ20170208_ct1.zip 20180215CCHSIO 49NZ20170208_nc_ctd.zip 20180215CCHSIO :Updated parameters: CTDPRS,CTDTMP,CTDSAL,CTDSVLSAL,CTDOXY,CTDFLUOR,CTDXMISS,CTDXMISSCP,CTDTURB, CTDPAR,CTDCDOMF opened in JOA with no apparent problems for the netcdf file 49NZ20170208_nc_ctd.zip. JOA did not properly display the full depth for the file 49NZ20170208_ct1.zip, probably becuase CTDPRS_FLAG_W is present. opened in ODV with no apparent problems: 49NZ20170208_ct1.zip • File Online Carolina Berys AL5400_POC_P17E.xlsx (download) #fbde0 Date: 2017-11-01 Current Status: unprocessed • File Online Carolina Berys Boss 06-22 report.xlsx (download) #a95fc Date: 2017-11-01 Current Status: unprocessed • File Online Carolina Berys MR16-09Leg3_recal_post_pco2_cal_v511.csv (download) #a775b Date: 2017-11-01 Current Status: unprocessed • File Online Carolina Berys mr2016_20160120.map.jpg (download) #e4fd9 Date: 2017-11-01 Current Status: unprocessed • File Online Carolina Berys sfcmet.zip (download) #8fff5 Date: 2017-11-01 Current Status: unprocessed • File Submission Carolina for Robert Key sfcmet.zip (download) #8fff5 Date: 2017-11-01 Current Status: unprocessed Notes Downloaded 2017-10-25 from http://www.jamstec.go.jp/iorgc/ocorp/data/p17erev_2017/index.html • File Submission Carolina for Robert Key mr2016_20160120.map.jpg (download) #e4fd9 Date: 2017-11-01 Current Status: unprocessed Notes Downloaded 2017-10-25 from http://www.jamstec.go.jp/iorgc/ocorp/data/p17erev_2017/index.html • File Submission Carolina for Robert Key MR16-09Leg3_recal_post_pco2_cal_v511.csv (download) #a775b Date: 2017-11-01 Current Status: unprocessed Notes Downloaded 2017-10-25 from http://www.jamstec.go.jp/iorgc/ocorp/data/p17erev_2017/index.html • File Submission Carolina for Robert Key Boss 06-22 report.xlsx (download) #a95fc Date: 2017-11-01 Current Status: unprocessed Notes Downloaded 2017-10-25 from http://www.jamstec.go.jp/iorgc/ocorp/data/p17erev_2017/index.html • File Submission Carolina for Robert Key AL5400_POC_P17E.xlsx (download) #fbde0 Date: 2017-11-01 Current Status: unprocessed Notes Downloaded 2017-10-25 from http://www.jamstec.go.jp/iorgc/ocorp/data/p17erev_2017/index.html • File Online Carolina Berys Cruise_Report_MR16-09_20170725.pdf (download) #64290 Date: 2017-11-01 Current Status: merged • File Submission Robert Key Cruise_Report_MR16-09_20170725.pdf (download) #64290 Date: 2017-10-25 Current Status: merged Notes Cruise Report here. Other files sent here and to Alex at NCEI via e-mail. See details in that message • File Online Carolina Berys 49NZ20170208_ct1.zip (download) #4454c Date: 2017-04-12 Current Status: merged • File Online Carolina Berys 49NZ20170208_sum.txt (download) #bbf13 Date: 2017-04-12 Current Status: unprocessed • File Submission see 49NZ20170208_sum.txt (download) #bbf13 Date: 2017-04-04 Current Status: unprocessed Notes Submitted for Katsuro Katsumata at JAMSTEC Final SUM and CTD files Dates: Feb 8 - Mar 5 2017 SHIP: Marai ChSci: Hiroshi Uchida Lines: P17E, P17S Collections: Pacific, SOCCOM, Southern? aliases MR16-09 Expocode 49NZ20170208 • File Submission see 49NZ20170208_ct1.zip (download) #4454c Date: 2017-04-04 Current Status: merged Notes Submitted for Katsuro Katsumata at JAMSTEC Final SUM and CTD files Dates: Feb 8 - Mar 5 2017 SHIP: Marai ChSci: Hiroshi Uchida Lines: P17E, P17S Collections: Pacific, SOCCOM, Southern? aliases MR16-09 Expocode 49NZ20170208