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太陽電波の観測と二三の考察
http://hdl.handle.net/2237/21745
http://hdl.handle.net/2237/2174565edc220-7aeb-4e30-8ae6-227d93f0c8a2
名前 / ファイル | ライセンス | アクション |
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Item type | 紀要論文 / Departmental Bulletin Paper(1) | |||||
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公開日 | 2015-04-28 | |||||
タイトル | ||||||
タイトル | 太陽電波の観測と二三の考察 | |||||
言語 | ja | |||||
その他のタイトル | ||||||
その他のタイトル | DATA ON SOLAR RADIO EMISSION WITH SOME NOTES | |||||
言語 | en | |||||
著者 |
柿沼, 隆清
× 柿沼, 隆清× 高柳, 利男× 太陽電波研究室一同× Kakinuma, Takakiyo× Takayanagi, Toshio× other members of Radio Astronomy Section |
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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 | The results of observations by 3750 and 9400 Mc/s radiometers are tabulated. The daily flux density at both frequencies has a correlation coefficient of 0.95, and the S-component at 9400 Mc/s is 0.8 times as large as that at 3750 Mc/s. The sense of polarization at both frequencies is similar. The percentage polarization referring to the S-component of an isolated radio spot occasionally exceeds 30 percent at 9400 Mc/s, which is much larger than that at 3750 Mc/s. Some bursts show yet a remarkable structure of frequency spectrum at these super-high-frequencies. The observations with an 8-element interferometer have been made for five hours every day for locating sources of outstanding occurrences. A burst occasionally occurs in an emissive region where no intense radiation is usually observed. | |||||
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 7, 号 1-2, p. 66-99, 発行日 1957-05-25 |
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値 | publisher | |||||
URI | ||||||
識別子 | http://hdl.handle.net/2237/21745 | |||||
識別子タイプ | HDL |