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  1. F300 宇宙地球環境研究所
  2. F300b 紀要
  3. 空電研究所報告
  4. 12(1-2)

太陽活動最盛期附近におけるマイクロ波太陽電波の静かな太陽成分について

http://hdl.handle.net/2237/21798
b8fa5f9e-c74c-41e4-9860-b0d74d7a8cd4
名前 / ファイル ライセンス アクション
bulria_12_1-2_15.pdf bulria_12_1-2_15.pdf (812.7 kB)
Item type 紀要論文 / Departmental Bulletin Paper(1)
公開日 2015-05-01
タイトル
タイトル 太陽活動最盛期附近におけるマイクロ波太陽電波の静かな太陽成分について
その他のタイトル
その他のタイトル QUIET SUN NEAR SUNSPOT MAXIMUM AT MICROWAVE FREQUENCY
著者 柿沼, 隆清

× 柿沼, 隆清

WEKO 57725

柿沼, 隆清

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KAKINUMA, Takakiyo

× KAKINUMA, Takakiyo

WEKO 57726

KAKINUMA, Takakiyo

Search repository
抄録
内容記述 From the observations with 4000 Mc/s interferometer, the flux density of the quiet sun component at 3750 Mc/s in 1957-58 is estimated at 122X10^-22W・m^-2(c/s)^-1. This value is about 1.6 times higher than the value at sunspot minimum. The recent interferometric observations suggest that the change of the quiet sun component at 9400 Mc/s during the sunspot cycle is only a few %. From the spectrum of the brightness of the center of the solar disk, derived from the eclipse observation at 9400, 3750, 2000 and 1000 Mc/s, the electron density of the corona around 1958 is estimated to be about 1.5-2.0 times higher than Alen-Baumbach' value.
内容記述タイプ Abstract
出版者
出版者 名古屋大学空電研究所
言語
言語 jpn
資源タイプ
資源 http://purl.org/coar/resource_type/c_6501
タイプ departmental bulletin paper
ISSN(print)
収録物識別子タイプ ISSN
収録物識別子 0465-7756
書誌情報 空電研究所報告

巻 12, 号 1-2, p. 15-18, 発行日 1962-03-25
著者版フラグ
値 publisher
URI
識別子 http://hdl.handle.net/2237/21798
識別子タイプ HDL
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