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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
http://hdl.handle.net/2237/21798b8fa5f9e-c74c-41e4-9860-b0d74d7a8cd4
名前 / ファイル | ライセンス | アクション |
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bulria_12_1-2_15.pdf (812.7 kB)
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Item type | 紀要論文 / Departmental Bulletin Paper(1) | |||||
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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 | |||||
言語 | ja | |||||
その他のタイトル | ||||||
その他のタイトル | QUIET SUN NEAR SUNSPOT MAXIMUM AT MICROWAVE FREQUENCY | |||||
言語 | en | |||||
著者 |
柿沼, 隆清
× 柿沼, 隆清× KAKINUMA, Takakiyo |
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アクセス権 | ||||||
アクセス権 | open access | |||||
アクセス権URI | http://purl.org/coar/access_right/c_abf2 | |||||
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. | |||||
言語 | en | |||||
内容記述タイプ | Abstract | |||||
出版者 | ||||||
言語 | ja | |||||
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 | |||||
出版タイプ | ||||||
出版タイプ | VoR | |||||
出版タイプResource | http://purl.org/coar/version/c_970fb48d4fbd8a85 | |||||
ISSN(print) | ||||||
収録物識別子タイプ | PISSN | |||||
収録物識別子 | 0465-7756 | |||||
書誌情報 |
ja : 空電研究所報告 巻 12, 号 1-2, p. 15-18, 発行日 1962-03-25 |
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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 |