*Kenta Ueki1, Minami Kazuki2, Tsuyoshi Iizuka3, Sanshiro Enomoto4, Hiroyuki Tanaka2 (1.Japan Agency for Marine-Earth Science and Technology, 2.Earthquake Research Institute, University of Tokyo, 3.Department of Earth and Planetary Science, University of Tokyo, 4.Center for Experimental Nuclear Physics and Astrophysics, University of Washington)
Session information
[E] Poster
S (Solid Earth Sciences ) » S-IT Science of the Earth's Interior & Techtonophysics
[S-IT21] Interaction and Coevolution of the Core and Mantle in the Earth and Planets
Mon. May 27, 2019 5:15 PM - 6:30 PM Poster Hall (International Exhibition Hall8, Makuhari Messe)
convener:Kenji Kawai(Department of Earth and Planetary Science, School of Science, University of Tokyo), Tsuyoshi Iizuka(University of Tokyo), Kenji Ohta(Department of Earth and Planetary Sciences, Tokyo Institute of Technology), Taku Tsuchiya(Geodynamics Research Center, Ehime University)
Recent observational and experimental investigations have significantly advanced our understanding of the structure and constituent materials of the deep Earth. Yet, even fundamental properties intimately linked with formation and evolution of the planet, such as details of the chemical heterogeneity in the mantle and light elements dissolved in the core, remained unclear. Seismological evidence has suggested a vigorous convection in the lower mantle, whereas geochemistry has suggested the presence of stable regions there that hold ancient chemical signatures. The amounts of radioactive isotopes that act as heat sources and drive dynamic behaviors of the deep Earth are also still largely unknown. We provide an opportunity to exchange the achievements and ideas, and encourage persons who try to elucidate these unsolved issues of the core-mantle evolution using various methods, including high-pressure and high-temperature experiments, high-precision geochemical and paleomagnetic analyses, high-resolution geophysical observations, geo-neutrino observations, and large-scale numerical simulations. Papers stimulating an interdisciplinary collaboration relating to establishment of the Japan-SEDI community are also welcomed.
[SIT21-P02] Towards a better estimation of the temperature distribution beneath the Japanese Islands
*Akiko Tanaka1, Makoto Yamano2, Hideki Hamamoto3, Shusaku Goto4, Takumi Matsumoto5 (1.Geological Survey of Japan, National Institute of Advanced Industrial Science and Technology, 2.Earthquake Research Institute, The University of Tokyo, 3.Center for Environmental Science in Saitama, 4.Institute for Geo-Resources and Environment National Institute of Advanced Industrial Science and Technology, 5.National Research Institute for Earth Science and Disaster Resilience)
*Satoru Haraguchi1, Kenta Ueki1, Hikaru Iwamori1,2,3 (1.Japan Agency for Marine-Earth Science and Technology, 2.Earthquake Research Institute, the University of Tokyo, 3.Tokyo Institute of Technology)
*Akio Suzuki1 (1.Department of Earth Science, Graduate School of Science, Tohoku University)
*seiji kimura1, Kenji Ohta6, Takaaki Kawazoe2, Kei Hirose3, Hiroyuki Kagi4, Takashi Yagi5 (1.Department of Earth and Planetary Sciences Tokyo Institute of Technology, 2.Department of Earth and Planetary Systems Science, Hiroshima University, 3.Earth-Life Science Institute, Tokyo Institute of Technology, 4.Geochemical Research Center, Graduate School of Science, University of Tokyo, 5.National Institute of Advanced Industrial Science and Technology, 6.Department of Earth and Planetary Sciences, Tokyo Institute of Technology)
*Tomoaki Kubo1, Moriyama Kazuya1, Yuichiro Mori1, Masahiro Imamura1, Sanae Koizumi2, Yu Nishihara3, Akio Suzuki4, Yuji Higo5 (1.Kyushu Univ., 2.ERI, 3.GRC Ehime Univ., 4.Tohoku Univ., 5.JASRI)
*YAMAMOTO TOMONARI1, Kenji Ohta1, Sho Suehiro1, Hayato Inoue1 (1.Tokyo Institute of Technology)
*Daisuke Yamazaki1, Noriyoshi Tsujino1, Yu Nishihara2 (1.Institute for Planetary Materials, Okayama University, 2.GRC, Ehime University)
*Kotaro Onga1, Kenji Ohta1, Akira Hasegawa1,2, Takashi Yagi2, Kei Hirose3,4, Yasuo Ohishi5 (1.Department of Earth and Planetary Sciences, Tokyo Institute of Technology, 2.National Institute of Advanced Industrial Science and Technology, 3.Earth-Life Science Institute, Tokyo Institute of Technology, 4.Department of Earth and Planetary Science, The University of Tokyo, 5.Japan Synchrotron Radiation Research Institute)
*Masayuki Nishi1,2, Koichiro Yamamoto1, Youmo Zhou1, Tetsuo Irifune2,1 (1.Geodynamics Research Center, Ehime University, 2.Earth-Life Science Institute, Tokyo Institute of Technology)
*Akira Hasegawa1,2, Kenji Ohta2, Takashi Yagi1, Kei Hirose3,4 (1.National Institute of Advanced Industrial Science and Technology, 2.Tokyo Institude of Technology, 3.Earth-Life Science Institute, Tokyo Institude of Technology, 4.The University of Tokyo)
*Satoru Tanaka1 (1.Department of Deep Earth Structure and Dynamics Research Japan Agency for Marine-Earth Science and Technology)
*Yuki Suzuki1, Kenji Kawai1, Robert J. Geller1, Satoru Tanaka2, Weerachai Siripuvaraporn3, Songkhun Boonchaisuku3, Noisagool Sutthipong3, Yasushi Ishihara2, Taweoon Kim, Koji MIYAKAWA4, Nozomu Takeuchi4 (1.The University of Tokyo, 2.Japan Agency for Marine-Earth Science and Technology, 3.Mahidol University, 4.Earthquake Research Institute, The University of Tokyo)
[SIT21-P14] Possible interaction between the core and mantle inferred from a core surface flow model
*Masaki Matsushima1 (1.Department of Earth and Planetary Sciences, School of Science, Tokyo Institute of Technology)
*Tomotaka Tanaka1, Hideharu Kuwahara2, Satoshi Kishi1, Ryuichi Nomura3, Kenji Mibe5, Hiroyuki Kagi4, Shigehiko Tateno6, Hirochika Sumino1 (1.Department of Basic Science, Graduate School of Arts and Sciences, The University of Tokyo , 2.Geodynamics Research Center, Ehime University, 3.Kyoto University, 4.Geochemical Research Center, Graduate School of Science, University of Tokyo, 5.Earthquake Research Institute, University of Tokyo, 6.Earth-Life Science Institute, Tokyo Institute of Technology)
*Innocent Ezenwa1, Takashi Yoshino1 (1.Institute for Planetary Materials, Okayama University)
*Norikatsu Akizawa1, Akira Ishikawa2, Katsuhiko Suzuki3, Tetsu Kogiso4 (1.Atmosphere and Ocean Research Institute, The University of Tokyo, 2.Department of Earth and Planetary Sciences, Tokyo Institute of Technology, 3.Research and Development Center for Submarine Resources, Japan Agency for Marine-Earth Science and Technology (JAMSTEC), 4.Graduate School of Human and Environmental Studies, Kyoto University)
*Atsuroh Ohba1, Taku Tsuchiya1 (1.Ehime University Geodynamics Research Center)
*Madhusoodhan Satish-Kumar1, Shinnosuke Aoyama1 (1.Department of Geology, Faculty of Science, Niigata University)
*Hayato Inoue1, Sho Suehiro1, Kenji Ohta1, Kei Hirose2,3, Yasuo Ohishi4 (1.Department of Earth and Planetary Sciences, Tokyo Institute of Technology, 2.Earth-Life Science Institute, Tokyo Institute of Technology, 3.Department of Earth and Planetary Science, The University of Tokyo, 4.Japan Synchrotron Radiation Research Institute)
[SIT21-P21] Electrical resistivity and thermal conductivity of fcc Fe: Implications for the Mercury’s core
★Invited Papers
*Hitoshi Gomi1, Takashi Yoshino1 (1.Okayama University)
*Toshiki Ohtaki1, Satoshi Kaneshima2, Taku Tsuchiya3 (1.Geological Survey of Japan, National Institute of Advanced Industrial Science and Technology (AIST), 2.Department of Earth and Planetary Sciences, Kyushu University, 3.Geodynamics Research Center, Ehime University)
*Shin-ichi Takehiro1, Youhei SASAKI2 (1.Research Institute for Mathematical Sciences, Kyoto University, 2.Department of Mathematics, Kyoto University)
*Ryohei Iritani1, Hitoshi Kawakatsu1, Nozomu Takeuchi1 (1.Earthquake Research Institute, Univ. of Tokyo)
*Haruhiko Dekura1, Taku Tsuchiya1 (1.Geodynamics Research Center, Ehime University)