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4,000MC帶における太陽面上の輻射強度分布について
http://hdl.handle.net/2237/21636
http://hdl.handle.net/2237/2163611fe3d43-ba91-434b-9cca-6e5003495670
名前 / ファイル | ライセンス | アクション |
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bulria_4_1_36.pdf (618.2 kB)
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Item type | 紀要論文 / Departmental Bulletin Paper(1) | |||||
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公開日 | 2015-04-21 | |||||
タイトル | ||||||
タイトル | 4,000MC帶における太陽面上の輻射強度分布について | |||||
言語 | ja | |||||
その他のタイトル | ||||||
その他のタイトル | ON THE DISTRIBUTION OF RADIO BRIGHTNESS ON THE SOLAR DISK AT ABOUT 4,000 MC | |||||
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 eclipse observation on Feb. 14, 1953, it is concluded that the radio solar disk is about 1.06 times larger than the optical disk. While,experimental record pattern,obtained from the interferometer,do not agree with the calculated one corresponding to uniform distribution over the radio disk. Experimental pattern is obtained if the excess region is about 2.5 times brighter than the optical disk of the uniform temperature,about 1.9x10^4°K. This assumption can also fully explain the variation of radio intensities in the later part of the eclipse when no active zones are covered. | |||||
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 4, 号 1, p. 36-38, 発行日 1953-09-25 |
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著者版フラグ | ||||||
値 | publisher | |||||
URI | ||||||
識別子 | http://hdl.handle.net/2237/21636 | |||||
識別子タイプ | HDL |