*Takuo Okuchi¹, Toshimori Sekine² (1.Institute for Planetary Materials, Okayama University, 2.Center for High Pressure Science and Technology Advanced Research)

*Tomoko Sato¹, Yoshinori Tange², Yusuke Seto³, Toshimori Sekine^4,5, Norimasa Ozaki⁴, Toyohito Nishikawa⁴, Kohei Miyanishi⁴, Kensuke Matsuoka⁴, Ryosuke Kodama⁴, Tadashi Togashi², Yuichi Inubushi², Toshinori Yabuuchi⁶, Makina Yabashi⁶ (1.Hiroshima University, 2.Japan Synchrotron Radiation Research Institute, 3.Kobe University, 4.Osaka University, 5.Center for High Pressure Science &Technology Advanced Research, 6.RIKEN)

*Tsubasa Tobase¹, Toshimori Sekine¹, Ginga Kitahara², Makoto Tokuda², Akira Yoshiasa², Makoto Takafuji², Tsutomu Mashimo², Nobuaki Kawai² (1.HPSTAR, 2.Graduate School of Science and Technology, Kumamoto University)

*Chi Pui Tang¹, Pak Kin Leong¹, Toshimori Sekine^2,3 (1.State Key Laboratory of Lunar and Planetary Sciences, Macau University of Science and Technology, 2.Center for High Pressure Science and Technology Advanced Research (HPSTAR) Shanghai Laboratory of HPSTAR, Shanghai, P.R. China, 3.Graduate School of Engineering, Osaka University)

*Takuo Okuchi¹, Toshimori Sekine² (1.Institute for Planetary Materials, Okayama University, 2.Center for High Pressure Science and Technology Advanced Research)

*Tomoko Sato¹, Yoshinori Tange², Yusuke Seto³, Toshimori Sekine^4,5, Norimasa Ozaki⁴, Toyohito Nishikawa⁴, Kohei Miyanishi⁴, Kensuke Matsuoka⁴, Ryosuke Kodama⁴, Tadashi Togashi², Yuichi Inubushi², Toshinori Yabuuchi⁶, Makina Yabashi⁶ (1.Hiroshima University, 2.Japan Synchrotron Radiation Research Institute, 3.Kobe University, 4.Osaka University, 5.Center for High Pressure Science &Technology Advanced Research, 6.RIKEN)

*Tsubasa Tobase¹, Toshimori Sekine¹, Ginga Kitahara², Makoto Tokuda², Akira Yoshiasa², Makoto Takafuji², Tsutomu Mashimo², Nobuaki Kawai² (1.HPSTAR, 2.Graduate School of Science and Technology, Kumamoto University)

*Chi Pui Tang¹, Pak Kin Leong¹, Toshimori Sekine^2,3 (1.State Key Laboratory of Lunar and Planetary Sciences, Macau University of Science and Technology, 2.Center for High Pressure Science and Technology Advanced Research (HPSTAR) Shanghai Laboratory of HPSTAR, Shanghai, P.R. China, 3.Graduate School of Engineering, Osaka University)

*Takuo Okuchi¹, Narangoo Purevjav¹, Norimasa Ozaki², Takeshi Matsuoka², Yusuke Seto³, Yoshinori Tange⁴, Toshinori Yabuuchi⁵, Naotaka Tomioka⁶, Toshimori Sekine⁷, Ryosuke Kodama² (1.Institute for Planetary Materials, Okayama University, 2.Graduate School of Engineering, Osaka University, 3.Graduate School of Science, Kobe University, 4.Japan Synchrotron Radiation Research Institute, 5.RIKEN Harima Branch, 6.Kochi Institute for Core Sample Research, Japan Agency for Marine-Earth Science and Technology, 7.Center for High Pressure Science and Technology Advanced Research)

*Yuhei Umeda¹, Norimasa Ozaki¹, Toshimori Sekine², Bruno Albertazzi³, Alessandra Benuzzi-Mounaix³, Riccardo Bolis³, Marco Guaruaglini³, Kento Katagiri¹, Kodama Ryosuke¹, Michel Koeing³, Kohei Miyanishi⁴, Shintaro Morioka¹, Toyohito Nishikawa¹, Syugo Ohi⁵, Alessandra Ravasio³, Yoichi Sakawa⁴, Takayoshi Sano⁴, Tomoko Sato⁶ (1.Graduate School of Engineering, Osaka Univ., 2.Center for High Pressure Science & Technology Advanced Research, 3.Ecole Polytechnique, 4.Institute of Laser Engineering, Osaka University, 5.Shiga Univ., 6.Graduate School of Science, Hiroshima University)

*Masahiro KAYAMA¹, Eiji Ohtani¹, Masaaki Miyahara², Shohei Kaneko¹, Toshimori Sekine³, Shin Ozawa¹, Naohisa Hirao⁴ (1.Tohoku University, 2.Hiroshima University, 3.HPSTAR, 4.Japan Synchrotron Radiation Research Institute)

*Masahiro KAYAMA¹, Eiji Ohtani¹, Masaaki Miyahara², Shohei Kaneko¹, Toshimori Sekine³, Shin Ozawa¹, Naohisa Hirao⁴ (1.Tohoku University, 2.Hiroshima University, 3.HPSTAR, 4.Japan Synchrotron Radiation Research Institute)