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A HIGH-RESOLUTION QUICK-SCAN INTERFEROMETER FOR SOLAR STUDIES AT 3.75 GHz
http://hdl.handle.net/2237/22009
http://hdl.handle.net/2237/22009aea84946-4c6b-490b-8f98-5654e2b47799
名前 / ファイル | ライセンス | アクション |
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proria_16_113.pdf (1.7 MB)
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Item type | 紀要論文 / Departmental Bulletin Paper(1) | |||||
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公開日 | 2015-05-25 | |||||
タイトル | ||||||
タイトル | A HIGH-RESOLUTION QUICK-SCAN INTERFEROMETER FOR SOLAR STUDIES AT 3.75 GHz | |||||
言語 | en | |||||
著者 |
TANAKA, Haruo
× TANAKA, Haruo× KAKINUMA, Takakiyo× ENOME, Shinzo× TORII, Chikayoshi× TSUKIJI, Yoshio× KOBAYASHI, Shoji |
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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 (32+2)-element compound interferometer for solar observations at 3.75 GHz has been in operation since August 1967. The HPBW is 23 seconds of arc for the compound and 1.1 minutes of arc for the 32-element adding interferometer. The outputs of these two kinds of interferometers are recorded at the same time with the sum and difference channels of two circularly polarized components. Artificial scanning of once each ten seconds by the adding interferometer has become possible since August 1968 for the observation of the rapidly changing burst. | |||||
言語 | en | |||||
内容記述タイプ | Abstract | |||||
出版者 | ||||||
言語 | en | |||||
出版者 | The Research Institute of Atmospherics, Nagoya University | |||||
言語 | ||||||
言語 | eng | |||||
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 | 0077-264X | |||||
書誌情報 |
en : Proceedings of the Research Institute of Atmospherics, Nagoya University 巻 16, p. 113-126, 発行日 1969-03-30 |
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著者版フラグ | ||||||
値 | publisher | |||||
URI | ||||||
識別子 | http://hdl.handle.net/2237/22009 | |||||
識別子タイプ | HDL |