論文

査読有り
2005年

Cosmic ray H-1 and H-2 spectra from BESS 98

MARS INTERNATIONAL REFERENCE ATMOSPHERE, LIVING WITH A STAR AND FUNDAMENTAL PHYSICS
  • ZD Myers
  • ES Seo
  • JZ Wang
  • RW Alford
  • K Abe
  • K Anraku
  • Y Asaoka
  • M Fujikawa
  • M Imori
  • T Maeno
  • Y Makida
  • H Matsumoto
  • H Matsunaga
  • J Mitchell
  • T Mitsui
  • A Moiseev
  • M Motoki
  • J Nishimura
  • M Nozaki
  • S Orito
  • J Ormes
  • T Saeki
  • T Sanuki
  • M Sasaki
  • Y Shikaze
  • T Sonoda
  • R Streitmatter
  • J Suzuki
  • K Tanaka
  • Ueda, I
  • N Yajima
  • T Yamagami
  • A Yamamoto
  • T Yoshida
  • K Yoshimura
    • … 全て表示
折りたたむ
巻
35
号
1
開始ページ
151
終了ページ
155
記述言語
英語
掲載種別
研究論文（学術雑誌）
DOI
10.1016/j.asr.2003.10.050
出版者・発行元
PERGAMON-ELSEVIER SCIENCE LTD
The Balloon-borne Experiment with a Super-solenoidal Spectrometer (BESS) instrument has been flown annually from Lynn Lake Manitoba since 1993. The instrument has been upgraded several times to improve its performance. The instalment flown in 1998 was able to detect H-2 clearly between 0.13 and 1.78 GeV/n as a result of improvements made on the time-of-flight (TOF) system. The BESS 98 data were analyzed to obtain the ratio and absolute fluxes of H-1 and H-2 over this energy range. The results were compared with different cosmic ray propagation models and their implications regarding their propagation history are discussed in this paper. (c) 2004 COSPAR. Published by Elsevier Ltd. All rights reserved.
リンク情報
DOI
https://doi.org/10.1016/j.asr.2003.10.050
Web of Science
https://gateway.webofknowledge.com/gateway/Gateway.cgi?GWVersion=2&SrcAuth=JSTA_CEL&SrcApp=J_Gate_JST&DestLinkType=FullRecord&KeyUT=WOS:000230948100024&DestApp=WOS_CPL
ID情報
  • DOI : 10.1016/j.asr.2003.10.050
  • ISSN : 0273-1177
  • Web of Science ID : WOS:000230948100024
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