Solar Gamma-Ray Lines and Interplanetary Solar Protons

• Yoshimori Masato

  Department of Physics, Faculty of Science, Rikkyo University

書誌事項

タイトル別名

• Solar Gamma Ray Lines and Interplanetar

抄録

Solar gamma-ray lines and protons were simultaneously observed for six flares on 1 April, 4 April, 27 April, 13 May 1981, 1 Feb., and 6 June, 1982 by Hinotori and Himawari satellites. The flare list is presented in Table I and the time histories of gamma-rays and protons are shown in Figs. 1 to 6. The relation-ship between the gamma-ray line fluences and peak proton fluxes for these flares is shown in Fig. 7. It does not reveal an apparent correlation between them. The present results imply that the protons producing gamma-ray lines in the flare region and protons observed near the Earth do not always belong to the same population, and favor the downward streaming model for the gamma-ray line production.

収録刊行物

• Ｊｏｕｒｎａｌ　ｏｆ　ｔｈｅ　Ｐｈｙｓｉｃａｌ　Ｓｏｃｉｅｔｙ　ｏｆ　Ｊａｐａｎ

  Ｊｏｕｒｎａｌ　ｏｆ　ｔｈｅ　Ｐｈｙｓｉｃａｌ　Ｓｏｃｉｅｔｙ　ｏｆ　Ｊａｐａｎ 54 (3), 1205-1213, 1985

  一般社団法人 日本物理学会

キーワード

• General Physics and Astronomy

詳細情報

• CRID: 1390001204183730304
• NII論文ID: 210000091933
• NII論文ID: 110001967296
• NII論文ID: 130003739379
• NII書誌ID: AA00704814
• DOI: 10.1143/jpsj.54.1205
• BIBCODE: 1985JPSJ...54.1205Y
• ISSN: 13474073
• ISSN: 00319015
• NDL書誌ID: 3015252
• Web Site: https://ndlsearch.ndl.go.jp/books/R000000004-I3015252
• Web Site: http://journals.jps.jp/doi/pdf/10.1143/JPSJ.54.1205
• 本文言語コード: en
• データソース種別:
  • JaLC
  • NDL
  • Crossref
  • CiNii Articles
• 抄録ライセンスフラグ: 使用不可