L
Lembit Sihver
Researcher at Vienna University of Technology
Publications - 167
Citations - 4845
Lembit Sihver is an academic researcher from Vienna University of Technology. The author has contributed to research in topics: Cosmic ray & Nucleon. The author has an hindex of 27, co-authored 158 publications receiving 4062 citations. Previous affiliations of Lembit Sihver include Purdue University & University of Fukui.
Papers
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Journal ArticleDOI
Features of Particle and Heavy Ion Transport code System (PHITS) version 3.02
Tatsuhiko Sato,Yosuke Iwamoto,Shintaro Hashimoto,Tatsuhiko Ogawa,Takuya Furuta,Shin ichiro Abe,Takeshi Kai,Pi En Tsai,Norihiro Matsuda,Hiroshi Iwase,Nobuhiro Shigyo,Lembit Sihver,Koji Niita +12 more
TL;DR: In this article, the Particle and Heavy Ion Transport Code System (PHITS) 3.02 has been released and the accuracy and the applicable energy ranges of the code were improved.
Journal ArticleDOI
Particle and Heavy Ion Transport code System, PHITS, version 2.52
Tatsuhiko Sato,Koji Niita,Norihiro Matsuda,Shintaro Hashimoto,Yosuke Iwamoto,Shusaku Noda,Tatsuhiko Ogawa,Hiroshi Iwase,Hiroshi Nakashima,Tokio Fukahori,Keisuke Okumura,Tetsuya Kai,Satoshi Chiba,Takuya Furuta,Lembit Sihver +14 more
TL;DR: An upgraded version of the Particle and Heavy Ion Transport code system (PHITS2.52) was developed and released to the public in this article, which is a more powerful tool for particle transport simulation applicable to various research and development fields.
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PHITS: A particle and heavy ion transport code system
Koji Niita,Tatsuhiko Sato,Hiroshi Iwase,Hiroyuki Nose,Hiroshi Nakashima,Lembit Sihver,Lembit Sihver +6 more
TL;DR: In this paper, the authors present a summary of the recent development of the multi-purpose Monte Carlo Particle and Heavy Ion Transport code system, PHITS, and discuss in detail the development of two new models, JAM and JQMD, for high energy particle interactions, incorporated in PHITS.
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Development of PARMA: PHITS based Analytical Radiation Model in the Atmosphere
TL;DR: An analytical model, named PARMA, is proposed for estimating the cosmic-ray spectra of neutrons, protons, helium ions, muons, electrons, positrons and photons applicable to any location in the atmosphere at altitudes below 20 km, that enables the cosmic radiation doses rapidly with a precision equivalent to that of the Monte Carlo simulation.
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Total reaction and partial cross section calculations in proton-nucleus (Zt <= 26) and nucleus-nucleus reactions (Zp and Zt <= 26).
TL;DR: In this paper, the authors developed semi-empirical total reaction cross section formulas for proton nucleus and nucleus-nucleus reactions for incident energies above 15 MeV and 100 MeV/nucleon respectively.