日本地球惑星科学連合2024年大会

セッション情報

[E] ポスター発表

セッション記号 S (固体地球科学) » S-IT 地球内部科学・地球惑星テクトニクス

[S-IT15] Mass and energy transport properties and processes in the crust and the mantle

2024年5月30日(木) 17:15 〜 18:45 ポスター会場 (幕張メッセ国際展示場 6ホール)

コンビーナ:Mysen Bjorn(Geophysical Laboratory, Carnegie Inst. Washington)、大谷 栄治(東北大学大学院理学研究科地学専攻)、高橋 菜緒子(東京大学大学院理学系研究科)、Codillo Emmanuel(Carnegie Institution for Science)



This session aims to present and discuss results of natural and laboratory observations together with theoretical modeling to describe mass and energy transport processes in the crust and the mantle. Magma and fluid are the main transport agents. Mass and heat transfer governed by magma and fluid mass and energy transport are imaged globally and locally by geophysical observations such as seismic tomography and electrical conductivity profiles.
Characterization of magma and fluid sources and the plumbing systems facilitating their formation, evolution, and movement in the mantle and crust rely on accurate chemical and physical property data. Transport properties of magma and fluid are characterized primarily by their composition, temperature, and pressure, which, in turn regulate element partitioning between minerals, magma, and fluid. Fluid abundance and composition in fluid-bearing environments also affects partial melting and crystallization processes together with physical properties including equation-of-state and rheology of magmatic systems. Transport processes governed by these chemical and physical properties include magma and fluid formation at depth and their ascent toward the surface.
The session will focus on those phenomena. Relevant information includes physical and chemical properties and processes of magma and fluid, as well as geophysical imaging and geochemical mapping of the Earth's interior at scales from local to global. Presentations can include results of laboratory experiments, numerical modeling, and observations using geophysical and geochemical approaches. Contributions to any of these subjects are encouraged. Commission of Physics of Minerals of the International Mineralogical Association (CPM-IMA) supports this session.

17:15 〜 18:45

*Yongsheng HUANG1,2、Guoji Wu1,2,3、Tatsumi Tsujimori4,5、Yuan Li1,2 (1.Guangzhou Institute of Geochemistry, Chinese Academy of Sciences, Guangzhou, China、2.CAS Center for Excellence in Deep Earth Science, Guangzhou, China、3.College of Earth and Planetary Sciences, University of the Chinese Academy of Sciences, Beijing, China、4.Department of Earth Science, Graduate School of Science, Tohoku University, Sendai, Japan 、5.Center for North Asian Studies, Tohoku University, Sendai, Japan)

17:15 〜 18:45

*Zhongiqng Wu1,2,3、Jiang Song1、Guochun Zhao4,5、Zhongxu Pan1 (1.Deep Space Exploration Laboratory / School of Earth and Space Sciences, University of Science and Technology of China, Hefei, Anhui, China.、2.CAS Center for Excellence in Comparative Planetology, University of Science and Technology of China, Anhui, China.、3.National Geophysical Observatory at Mengcheng, University of Science and Technology of China, Anhui, China.、4.Department of Earth Sciences, The University of Hong Kong, Hong Kong, Hong Kong、5.Department of Geology, State Key Laboratory of Continental Dynamics, Northwest University, Xi'an, China)

17:15 〜 18:45

*高市 合流1石井 貴之2西原 遊1松影 香子3肥後 祐司4辻野 典秀4柿澤 翔4 (1.愛媛大学地球深部ダイナミクス研究センター、2.岡山大学惑星物質研究所、3.帝京科学大学自然環境学科、4.(公財)高輝度光科学研究センター)

17:15 〜 18:45

*Jintao Zhu1,2,3Takayuki Ishii1、Renbiao Tao3、Lifei Zhang2 (1.Institute for Planetary Materials, Okayama University、2.MOE Key Laboratory of Orogenic Belts and Crustal Evolution, School of Earth and Space Sciences, Peking University、3.Center for High Pressure Science and Technology Advanced Research (HPSTAR))

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