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INTERPLANETETALY MANIFESTATION OF THE "HALO" CORONAL MASS EJECTION OF NOVEMBER 27, 1979
http://hdl.handle.net/2237/22115
http://hdl.handle.net/2237/2211520b7c18d-73c9-446f-9d68-5f2b1793bb58
名前 / ファイル | ライセンス | アクション |
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proria_32_11.pdf (3.0 MB)
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Item type | 紀要論文 / Departmental Bulletin Paper(1) | |||||
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公開日 | 2015-05-29 | |||||
タイトル | ||||||
タイトル | INTERPLANETETALY MANIFESTATION OF THE "HALO" CORONAL MASS EJECTION OF NOVEMBER 27, 1979 | |||||
言語 | en | |||||
著者 |
Watanabe, Takashi
× Watanabe, Takashi |
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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 | This paper presents a case study of a solar wind disturbance associated with the "halo" coronal mass ejection (CME) of November 27, 1979, which was a 360° coronal density enhancement encircling the occulting disk (Howard et al., 1982). The principal sources of solar wind data are spacecraft observations and IPS observations. The interplanetary manifestation of the CME was a quasi-spherical solar wind disturbance. The total angular spread was greater than 70° at 1 AU heliocentric distance in the longitudinal direction. | |||||
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 32, p. 11-28, 発行日 1985-03-25 |
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著者版フラグ | ||||||
値 | publisher | |||||
URI | ||||||
識別子 | http://hdl.handle.net/2237/22115 | |||||
識別子タイプ | HDL |