Solar flare and neutron telescope

Y. Muraki, Y. Matsubara, I. Imaida, T. Koi, T. Murata, A. Okada, S. Sakakibara, T. Sako, H. Tsuchiya, Y. Munakata, S. Shibata, R. Tatsuoka, H. Sakai, T. Nonaka, T. Ohnishi, T. Wakasa, K. Hatanaka, Y. Ishida

研究成果: Contribution to journalArticle査読

1 被引用数 (Scopus)

抄録

For the solar neutron event of June 3rd,1982, a new interpretation is given on ion acceleration mechanisms at the solar surface. The event can be explained by the impulsive acceleration of ions just after electron acceleration. For the June 4th,1991 solar neutron event, discrepancies in the absolute solar neutron fluxes measured by three different detectors are investigated using neutron beams at RCNP, Osaka university. We propose here an interpretation which explains all data consistently based on the premise that solar neutrons generate many low energy neutrons in the atmosphere by internuclear cascade processes.

本文言語英語
ページ(範囲)3-11
ページ数9
ジャーナルNuclear Physics B - Proceedings Supplements
60
3
DOI
出版ステータス出版済み - 1 1998
外部発表はい

All Science Journal Classification (ASJC) codes

  • 原子分子物理学および光学
  • 核物理学および高エネルギー物理学

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