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IGYにおけるマイクロ派太陽電波の観測
http://hdl.handle.net/2237/21755
http://hdl.handle.net/2237/21755c603fbee-30bc-4022-9356-3d945c86b398
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 | IGYにおけるマイクロ派太陽電波の観測 | |||||
言語 | ja | |||||
その他のタイトル | ||||||
その他のタイトル | OBSERVATIONS OF SOLAR RADIO EMISSION AT MICROWAVE FREQUENCIES FOR IGY | |||||
言語 | en | |||||
著者 |
田中, 春夫
× 田中, 春夫× 柿沼, 隆清× 神藤, 英彦× 高柳, 利男× 鳥居, 近吉× TANAKA, Haruo× 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 | Outline of the equipment used for solar radio observations at Toyokawa station which are in operation since the begining of IGY is described together with the method of tabulation. Percentage variation of the S-component versus frequency is calculated for the first half-year period of IGY, which shows a peak near 4000 Mc/s. Left-hand polarization of S-component prevails in this period at frequencies below 3750 Mc/s and there are many cases where the sense of polarization reverses between 3750 and 9400 Mc/s. Experiment has been made for detecting linear polarization at a frequency of 3750 ± 5 Mc/s, but we have yet no data to show the existence of linear polarization for both S-component and outstanding occurrences. | |||||
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 8, 号 1-2, p. 67-73, 発行日 1958-03-20 |
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著者版フラグ | ||||||
値 | publisher | |||||
URI | ||||||
識別子 | http://hdl.handle.net/2237/21755 | |||||
識別子タイプ | HDL |