MR11A:
Emulating Planetary Interiors in the Laboratory: Mineral Physics Experiments and Simulations I Posters

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Session ID#: 12383

Session Description:
We invite contributions describing recent advances in experiments and simulations on planetary materials: effects of high pressure, high temperature, or strain rates on equations of state, phase transformations, elasticity, transport properties, and their implications for understanding of the formation, structure, and evolution of the interior of the Earth and other planets.
Primary Convener:  Marius A Millot, Lawrence Livermore National Laboratory, Livermore, CA, United States
Conveners:  Marius A Millot, Lawrence Livermore National Laboratory, Livermore, CA, United States and Sebastien Merkel, Univ. Lille, Lille, France
Chairs:  Marius A Millot, Lawrence Livermore National Laboratory, Livermore, CA, United States and Sebastien Merkel, Univ. Lille, Lille, France
OSPA Liaison:  Sebastien Merkel, Univ. Lille, Lille, France

Cross-Listed:
  • DI - Study of the Earth's Deep Interior
  • P - Planetary Sciences
  • V - Volcanology, Geochemistry and Petrology
Index Terms:

3919 Equations of state [MINERAL PHYSICS]
3924 High-pressure behavior [MINERAL PHYSICS]
3944 Shock wave experiments [MINERAL PHYSICS]
3994 Instruments and techniques [MINERAL PHYSICS]

Abstracts Submitted to this Session:

Atsushi Kyono1, Masato Kato1, Asami Sano-Furukawa2, Shin-ichi Machida3 and Takanori Hattori4, (1)University of Tsukuba, Tsukuba, Japan, (2)JAEA Japan Atomic Energy Agency, Toki, Japan, (3)Comprehensive Research Organization for Science and Society, Neutron Science and Technology Center, Tokai, Japan, (4)Japan Atomic Energy Agency, Tokai, Japan
Tao Liu, University of Chinese Academy of Sciences, Beijing, China and Duojun Wang, UCAS University of Chinese Academy of Sciences, Beijing, China
Tian Qin1, Koichiro Umemoto2, Renata Wentzcovitch1, Marc M Hirschmann3 and David L Kohlstedt1, (1)University of Minnesota Twin Cities, Minneapolis, MN, United States, (2)Tokyo Institute of Technology, Earth-Life Science Institute, Tokyo, Japan, (3)University of Minnesota Twin Cities, Department of Earth and Environmental Sciences, Minneapolis, United States
Yu-Hsiang Chien1,2 and Wen-Pin Hsieh1, (1)Institute of Earth Sciences Academia Sinica, Taipei, Taiwan, (2)NCU National Central University of Taiwan, Earth System Science Program, Taiwan International Graduate Program (TIGP), Jhongli, Taiwan
Joseph R Smyth, University of Colorado Boulder, Department of Geological Sciences, Boulder, CO, United States, Takaaki Kawazoe, University of Bayreuth, Bayerisches Geoinstitut, Bayreuth, Germany and Li Zhang, University of Colorado at Boulder, Geological Sciences, Boulder, United States
Innocent Ezenwa1, Richard Secco2 and Wenjun Yong1, (1)University of Western Ontario, London, ON, Canada, (2)University of Western Ontario, Earth Sciences, London, ON, Canada
Reynold E Silber1, Richard Secco1 and Wenjun Yong2, (1)University of Western Ontario, Earth Sciences, London, ON, Canada, (2)University of Western Ontario, London, ON, Canada
Sho Suehiro, Tokyo Institute of Technology, Department of Earth and Planetary Sciences, Tokyo, Japan, Kenji Ohta, Institute of Science Tokyo, Department of Earth and Planetary Sciences, Tokyo, Japan, Takashi Yagi, AIST - National Institute of Advanced Industrial Science and Technology, Tsukuba, Japan and Kei Hirose, Tokyo Institute of Technology, Earth-Life Science Institute, Tokyo, Japan
Budhi K Godwal1, Kevin P Driver1, Raymond Jeanloz2 and Burkhard Militzer3, (1)University of California Berkeley, Berkeley, CA, United States, (2)University of California Berkeley, Earth and Planetary Science, Berkeley, CA, United States, (3)University of California Berkeley, Department of Astronomy, Berkeley, United States
Kevin P Driver1, Shuai Zhang1 and Burkhard Militzer2, (1)University of California Berkeley, Berkeley, CA, United States, (2)University of California Berkeley, Department of Astronomy, Berkeley, United States
Mu LI1,2, Shuai Zhang1, Raymond Jeanloz3 and Burkhard Militzer4, (1)University of California Berkeley, Berkeley, CA, United States, (2)CAEP China Academy of Engineering Physics, Institute of Fluid Physics, Mianyang, China, (3)University of California Berkeley, Earth and Planetary Science, Berkeley, CA, United States, (4)University of California Berkeley, Department of Astronomy, Berkeley, United States
Oleg V. Fat\'yanov, California Institute of Technology, Pasadena, CA, United States and Paul D Asimow, California Institute of Technology, Division of Geological and Planetary Sciences, Pasadena, CA, United States
Matthew R Diamond, University of California Berkeley, Berkeley, CA, United States, Raymond Jeanloz, University of California Berkeley, Earth and Planetary Science, Berkeley, CA, United States and Burkhard Militzer, University of California Berkeley, Department of Astronomy, Berkeley, United States
Marion Harmand1, Andrew Krygier2, Bruno Albertazzi3, Karen Appel4, Alessandra Benuzzi-Mounaix5, Emma E McBride6, Marco Cammarata7, Yiping Feng8, Eric Galtier6, Nicholas Hartley3, Ryosuke Kodama9, Zuzana Konopkova10, Hae Ja Lee6, Henrik T Lemke11, Guillaume Morard1, Koei Miyanishi3, Bob Nagler6, Ruidy Nemausat1, Norimasa Ozaki9, Toshimori Sekine12, Volodymyr Svitlyk13, Tommaso Vinci5, Diling Zhu8, Michel Koenig5 and Guillaume Fiquet14, (1)IMPMC Institut de Minéralogie et de Physique des Milieux Condensés, Paris Cedex 05, France, (2)Lawrence Livermore National Laboratory, Livermore, United States, (3)Osaka University, Osaka, Japan, (4)European XFEL, Schenefeld, Germany, (5)Ecole Polytechnique, LULI / CNRS, Palaiseau Cedex, France, (6)SLAC National Accelerator Laboratory, Menlo Park, United States, (7)Institut Physique de Rennes IPR - CNRS, Rennes, France, (8)SLAC National Accelerator Laboratory, Menlo Park, CA, United States, (9)Osaka University, Faculty of Engineering, Osaka, Japan, (10)DESY Deutsches Elektronen Synchrotron, Hamburg, Germany, (11)Paul Scherrer Institute, Villingen, Switzerland, (12)Hiroshima University, Higashi-Hiroshima, Japan, (13)ESRF European Synchrotron Radiation Facility, Grenoble, France, (14)Sorbonne Université - MNHN - CNRS - IMPMC, Paris, France
Takuo Okuchi1, Norimasa Ozaki2, Takayoshi Sano3, Youichi Sakawa3 and Ryosuke Kodama2,3, (1)Institute for Planetary Materials, Okayama University, Misasa, Tottori, Japan, (2)Osaka University, Faculty of Engineering, Osaka, Japan, (3)Osaka University, Institure of Laser Engineering, Osaka, Japan
Erik Davies, University of California Davis, Earth and Planetary Sciences, Davis, United States, Seth Root, Sandia National Laboratories, Albuquerque, United States, Dylan Spaulding, University of California Davis, Earth and Planetary Sciences, Davis, CA, United States, Richard G Kraus, Lawrence Livermore National Laboratory, Livermore, CA, United States, Sarah T Stewart, University of California, Earth and Planetary Sciences, Davis, United States, Stein B Jacobsen, Harvard University, Earth and Planetary Sciences, Cambridge, MA, United States and Thomas R Mattsson, Sandia National Laboratory, Albuquerque, NM, United States