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9400MCにおける太陽電波の観測
http://hdl.handle.net/2237/21734
http://hdl.handle.net/2237/217344aa6d2fc-56b8-4bea-9475-8c2df48c6ff9
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 | 2015-04-27 | |||||
タイトル | ||||||
タイトル | 9400MCにおける太陽電波の観測 | |||||
言語 | ja | |||||
その他のタイトル | ||||||
その他のタイトル | THE OBSERVATION OF SOLAR RADIO EMISSION AT 9,400 MC | |||||
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× JINDO, Hidehiko× TAKAYANAGI, Toshio× TORII, Chikayoshi |
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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 | A 1.2 meter dish radio telescope for use at 9,400 MC was completed at the end of 1955. A circular-waveguide feed at the focus of the dish is connected directly to a turnstile circuit and 4 polarized components can be received by switching. The Dicke's modulation is performed statically by the circulator using a Faraday plate, and the modulation frequency is 500 c/s. S-component at 9,400 MC is 30% of that observed at 3750 MC refering to each quiet level. On the logarithmic scale, the height of outstanding occurrences are almost the same at two frequencies. Some bursts observed in January and February 1956 have no connection with each other at two frequencies, which suggests that remarkable frequency spectrum still exists at these high frequencies. | |||||
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 6, 号 1-2, p. 61-66, 発行日 1956-04-25 |
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著者版フラグ | ||||||
値 | publisher | |||||
URI | ||||||
識別子 | http://hdl.handle.net/2237/21734 | |||||
識別子タイプ | HDL |