Y
Yoshio Suzuki
Researcher at Hitachi
Publications - 451
Citations - 8823
Yoshio Suzuki is an academic researcher from Hitachi. The author has contributed to research in topics: Zone plate & Synchrotron radiation. The author has an hindex of 42, co-authored 435 publications receiving 8256 citations. Previous affiliations of Yoshio Suzuki include Nihon University & University of Pennsylvania.
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Demonstration of X-Ray Talbot Interferometry
TL;DR: In this article, the first X-ray Talbot interferometry was demonstrated using a pair of transmission gratings made by forming gold stripes on glass plates, which were aligned on the optical axis of X-rays with a separation that caused the Talbot effect by the first grating.
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Phase Tomography by X-ray Talbot Interferometry for Biological Imaging
TL;DR: The X-ray phase tomography of biological samples is reported in this paper, which is based on Xray Talbot interferometry, and imaging results obtained for a cancerous rabbit liver and a mouse tail with synchrotron radiation are presented.
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Three-Dimensional Structure of Hayabusa Samples: Origin and Evolution of Itokawa Regolith
Akira Tsuchiyama,Masayuki Uesugi,Takashi Matsushima,Tatsuhiro Michikami,Toshihiko Kadono,Tomoki Nakamura,Kentaro Uesugi,Tsukasa Nakano,Scott A. Sandford,Ryo Noguchi,Toru Matsumoto,Junya Matsuno,Takashi Nagano,Y. Imai,Akihisa Takeuchi,Yoshio Suzuki,T. Ogami,Jun Katagiri,Mitsuru Ebihara,Trevor Ireland,Fumio Kitajima,Keisuke Nagao,Hiroshi Naraoka,Takaaki Noguchi,Ryuji Okazaki,Hisayoshi Yurimoto,Michael E. Zolensky,Toshifumi Mukai,Masanao Abe,Toru Yada,Akio Fujimura,Makoto Yoshikawa,Jun'ichiro Kawaguchi +32 more
TL;DR: Regolith particles on the asteroid Itokawa were recovered by the Hayabusa mission and their three-dimensional structure and other properties, revealed by x-ray microtomography, provide information on regolith formation.
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Bond-orientational anisotropy in metallic glasses observed by x-ray diffraction
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Elemental Compositions of Comet 81P/Wild 2 Samples Collected by Stardust
George J. Flynn,Pierre Bleuet,Janet Borg,John P. Bradley,Frank E. Brenker,Sean Brennan,John Bridges,Donald E. Brownlee,Emma S. Bullock,Manfred Burghammer,Benton C. Clark,Zu Rong Dai,Charles P. Daghlian,Zahia Djouadi,Sirine C. Fakra,T. Ferroir,Christine Floss,Ian A. Franchi,Zack Gainsforth,Jean-Paul Gallien,Philippe Gillet,Patrick G. Grant,Giles A. Graham,Simon F. Green,F. Grossemy,Philipp R. Heck,Gregory F. Herzog,Peter Hoppe,Friedrich Hörz,Joachim Huth,Konstantin Ignatyev,Hope A. Ishii,Koen Janssens,David J. Joswiak,Anton T. Kearsley,Hicham Khodja,Antonio Lanzirotti,Jan Leitner,Laurence Lemelle,Hugues Leroux,K. Luening,Glenn J. MacPherson,Kuljeet K. Marhas,Matthew A. Marcus,Graciela Matrajt,Tomoki Nakamura,Keiko Nakamura-Messenger,Tsukasa Nakano,Matthew Newville,D. A. Papanastassiou,Piero Pianetta,William Rao,Christian Riekel,Frans J. M. Rietmeijer,Detlef Rost,Craig S. Schwandt,Thomas H. See,Julie Sheffield-Parker,Alexandre Simionovici,Ilona Sitnitsky,Christopher J. Snead,Frank J. Stadermann,Thomas Stephan,Rhonda M. Stroud,Jean Susini,Yoshio Suzuki,Stephen R. Sutton,Susan Taylor,Nick Teslich,David Troadec,Peter Tsou,Akira Tsuchiyama,Kentaro Uesugi,Bart Vekemans,Edward P. Vicenzi,Laszlo Vincze,Andrew J. Westphal,Penelope J. Wozniakiewicz,Ernst Zinner,Michael E. Zolensky +79 more
TL;DR: The elements Cu, Zn, and Ga appear enriched in this Wild 2 material, which suggests that the CI meteorites may not represent the solar system composition for these moderately volatile minor elements.