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THE MOST INTENSE BURST OF SOLAR RADIO EMISSION OBSERVED ON FEBRUARY 23, 1956
http://hdl.handle.net/2237/21615
http://hdl.handle.net/2237/21615e1ffee85-1fba-4790-b312-c9b12e4e7633
| 名前 / ファイル | ライセンス | アクション |
|---|---|---|
Vol4-6.pdf (544.3 kB)
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| Item type | 紀要論文 / Departmental Bulletin Paper(1) | |||||
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| 公開日 | 2015-04-20 | |||||
| タイトル | ||||||
| タイトル | THE MOST INTENSE BURST OF SOLAR RADIO EMISSION OBSERVED ON FEBRUARY 23, 1956 | |||||
| 言語 | en | |||||
| 著者 |
TANAKA, HARUO
× 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 | ||||||
| 内容記述タイプ | Abstract | |||||
| 内容記述 | A violent outburst of solar radio emission was observed on February 23, 1956. A perfect record of the intensity was successfully obtained by 3750 and 9400 Mc/s radiometers, together with a drift curve taken by an 8-element interferometer at 4000 Mc/s. The maximum intensity was 225 and 141 times as large as that of the quiet-sun radiation for 3750 and 9400 Mc/s radio flux density, respectively. The position of the radio source at 4000 Mc/s slightly moved during the burst. The most probable E-W width of the radio source during the burst is 3 minutes of arc, which corresponds to the maximum effective temperature of about 5×10^8 K. | |||||
| 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 | ||||||
| 資源タイプ識別子 | http://purl.org/coar/resource_type/c_6501 | |||||
| 資源タイプ | 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 4, p. 74-77, 発行日 1957-03-25 |
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| 著者版フラグ | ||||||
| 値 | publisher | |||||
| URI | ||||||
| 識別子 | http://hdl.handle.net/2237/21615 | |||||
| 識別子タイプ | HDL | |||||
