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"Katsura, Tomoo*; Funakoshi, Kenichi*; Kubo, Atsushi*; Nishiyama, Norimasa*; Tange, Yoshinori*; Sueda, Yuichiro*; Kubo, Tomoaki*; Utsumi, Wataru
Physics of the Earth and Planetary Interiors, 143-144, p.497 - 506, 2004/06
Times Cited Count：109 Percentile：86.75(Geochemistry & Geophysics)no abstracts in English
Utsumi, Wataru; Katayama, Yoshinori; Saito, Hiroyuki; Kaneko, Hiroshi*; Okada, Taku*; Otaka, Osamu*
Mirai O Hiraku Koatsuryoku Kagaku Gijutsu Semina Shirizu, 28, p.14 - 20, 2004/01
no abstracts in English
Katsura, Tomoo*; Funakoshi, Kenichi*; Nishiyama, Norimasa*; Kubo, Atsushi*; Tange, Yoshinori*; Sueda, Yuichiro*; Kubo, Tomoaki*; Utsumi, Wataru
Hoshako, 16(6), p.352 - 357, 2003/11
no abstracts in English
under high pressure and high peratureOtaka, Osamu*; Fukui, Hiroyuki*; Kunisada, Taichi*; Fujisawa, Tomoyuki*; Funakoshi, Kenichi*; Utsumi, Wataru; Irifune, Tetsuo*; Kuroda, Koji*; Kikegawa, Takumi*
Physical Review B, 63(17), p.174108_1 - 174108_8, 2001/05
Times Cited Count：127 Percentile：96.62(Materials Science, Multidisciplinary)no abstracts in English
Utsumi, Wataru; Funakoshi, Kenichi*; Yagi, Naoto*; Urakawa, Satoru*; Otaka, Osamu*; Katsura, Tomoo*; Irifune, Tetsuo*; Inoue, Toru*; Uchida, Takeyuki*
Ganseki Kobutsu Kagaku, 30(2), p.100 - 101, 2001/03
no abstracts in English
Funakoshi, Kenichi*; Utsumi, Wataru; Otaka, Osamu*; Irifune, Tetsuo*; Inoue, Toru*; Ito, Eiji*; Katsura, Tomoo*; Kubo, Atsushi*; Hirose, Kei*; Ando, Junichi*; et al.
Ganseki Kobutsu Kagaku, 30(2), p.102 - 103, 2001/03
no abstracts in English
observation of ilmenite-perovskite phase transition in MgSiO
using synchrotron radiationOno, Shigeaki*; Katsura, Tomoo*; Ito, Eiji*; Kanzaki, Masami*; Yoneda, Akira*; Walter, M.*; Urakawa, Satoru*; Utsumi, Wataru; Funakoshi, Kenichi*
Geophysical Research Letters, 28(5), p.835 - 838, 2001/03
Times Cited Count：79 Percentile：86.2(Geosciences, Multidisciplinary)no abstracts in English
X-ray observation of cubic BCN formation under high pressures and temperaturesUtsumi, Wataru; Okada, Taku; Funakoshi, Kenichi*; Shimomura, Osamu
Proceeding of the 8th NIRIM International Symposium on Advanced Materials (ISAM 2001), p.39 - 40, 2001/03
no abstracts in English
Yamakata, Masaaki*; Mizutani, Takeshi; Utsumi, Wataru; Katayama, Yoshinori; Shimomura, Osamu
Science and Technology of High Pressure (Proceedings of AIRAPT-17), p.1109 - 1112, 2000/00
no abstracts in English
Utsumi, Wataru
Proceeding of the 3rd China-Japan High Pressure Conference, 6 Pages, 1998/00
no abstracts in English
Utsumi, Wataru; Funakoshi, Kenichi*; Urakawa, Satoru*; Yamakata, Masaaki*; Tsuji, Kazuhiko*; Konishi, Hiroyuki; Shimomura, Osamu
Review of High Pressure Science and Technology, 7, p.1484 - 1486, 1998/00
no abstracts in English
Hattori, Takanori; Sano, Asami; Machida, Shinichi*; Abe, Jun*; Funakoshi, Kenichi*
no journal, ,
Six-axis multi-anvil press ATSUHIME is the press installed at high-pressure neutron beamline PLANET in J-PARC. It was constructed for neutron diffraction experiments. At present, PLANET is only the beamline wherein high-pressure and high-temperature experiments are routinely conducted. Thus, the six-axis press has been used in a wide range of scientific fields, such as physics, geoscience, and physical chemistry. In this talk, I introduce the design and performance of the press as well as recent neutron studies conducted using ATSUHIME.
Sano, Asami
no journal, ,
Since hydrogen has a large scattering power for neutron, neutron diffraction can be an important tool in the investigation of hydrogen in minerals. The high-pressure neutron diffractometer PLANET in the MLF at J-PARC is equipped with a 6-axis type multi-anvil press to conduct high-temperature neutron diffraction experiments at high pressure. With the application of the multi-anvil assembly (MA) 6-6, experiments have been routinely performed. One of the advantages of using the MA6-6 is that the anvil gap is located at 2
= 90
, where the detector is located. However, the available pressure is currently limited below 12 GPa using MA6-6 with TEL size of 7 mm. It is necessary to expand the conditions to cover the mantle transition zone that is considered as an important reservoir of water. In this talk, I will present recent developments with applications of MA6-8 to expand the PT conditions in PLANET.
