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空電電界强度の異常増加について
http://hdl.handle.net/2237/21728
http://hdl.handle.net/2237/21728c6d7ff65-0f9e-4974-957f-7a75d1b36fa5
名前 / ファイル | ライセンス | アクション |
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bulria_6_1-2_21.pdf (2.0 MB)
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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 | 空電電界强度の異常増加について | |||||
言語 | ja | |||||
その他のタイトル | ||||||
その他のタイトル | ON THE SUDDEN ENHANCEMENT OF ATMOSPHERICS | |||||
言語 | en | |||||
著者 |
金原, 淳
× 金原, 淳× KIMPARA, Atsushi |
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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 | In the calm period of solar activity where only the solar flares of importance 1 occur, it is rather difficult to determine which flares among them are active enough to excite SEA in VLF range. The author investigated mainly in 1955 the correlation between SEA at 27, 21. and 10 kc and the outburst in solar radio waves at 3,750 Mc, and found that the stronger the outburst, the more distinctly SEA is observed, and in average the maximum intensity of 27 kc lags 6.4 minutes behind that of outburst while that of 21 kc leads 5.4 minutes, and both of them recovers to the normal value after the period of 20 minutes to more than 1 hour depending upon the intensity of outburst, and the intensity of 10 kc decreases for strong outburst and is indifferent to weak one. | |||||
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. 21-31, 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/2237/21728 | |||||
識別子タイプ | HDL |