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ON THE DISTRIBUTION OF RADIO BRIGHTNESS ON THE QUIET SOLAR DISK AT 4,000 MC/s
http://hdl.handle.net/2237/21568
http://hdl.handle.net/2237/215688b726611-c52d-4663-bd57-8be2269a2b76
| 名前 / ファイル | ライセンス | アクション |
|---|---|---|
Vol3-10.pdf (867.4 kB)
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| Item type | 紀要論文 / Departmental Bulletin Paper(1) | |||||
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| 公開日 | 2015-04-16 | |||||
| タイトル | ||||||
| タイトル | ON THE DISTRIBUTION OF RADIO BRIGHTNESS ON THE QUIET SOLAR DISK AT 4,000 MC/s | |||||
| 言語 | en | |||||
| 著者 |
KAKINUMA, TAKAKIYO
× 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 | ||||||
| 内容記述タイプ | Abstract | |||||
| 内容記述 | An 8 element interferometer with quarter-wavelength plates operating at 4,000 MC has been constructed and observations have been carried out since June 1954. The daily drift curves from June 1954 to June 1955 were superimposed at intervals of about one month and E-W one dimensional brightness distributions on the quiet sun were calculated from the lower envelopes of these curves. If circular symmetry is assumed, the derived radial brightness distributions show limb-brightening. | |||||
| 言語 | en | |||||
| 出版者 | ||||||
| 出版者 | The Research Institute of Atmospherics, Nagoya University | |||||
| 言語 | en | |||||
| 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 3, p. 96-101, 発行日 1956-01-30 |
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| 著者版フラグ | ||||||
| 値 | publisher | |||||
| URI | ||||||
| 識別子 | http://hdl.handle.net/2237/21568 | |||||
| 識別子タイプ | HDL | |||||
