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THE RADIAL EVOLUTION OF ENHANCED SCINTILLATION REGIONS
http://hdl.handle.net/2237/22088
http://hdl.handle.net/2237/22088fef55078-6e9a-4881-b3d5-891262e3226f
名前 / ファイル | ライセンス | アクション |
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Item type | 紀要論文 / Departmental Bulletin Paper(1) | |||||
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公開日 | 2015-05-28 | |||||
タイトル | ||||||
タイトル | THE RADIAL EVOLUTION OF ENHANCED SCINTILLATION REGIONS | |||||
言語 | en | |||||
著者 |
Houminer, Zwi
× Houminer, Zwi× Kojima, Masayoshi× 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 | Observations of scintillation index and solar wind velocity using a grid of sources at 327MHz, enable us to study the radial evolution of enhanced scintillation regions between 0.3-1.0 a.u. and at a large range of heliocentric latitudes. Statistical analysis as well as the study of specific events during the declining phase of the solar cycle, show that enhanced scintillation regions associated with compressed plasma density due to the interaction between fast and slow solar wind flows, develop only beyond 0.5 a.u. At distances less than 0.5 a.u., the scintillation index varies in a similar manner to the variations in plasma density as observed by space probes at the same distances from the Sun. | |||||
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 34, p. 1-8, 発行日 1987-03-25 |
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著者版フラグ | ||||||
値 | publisher | |||||
URI | ||||||
識別子 | http://hdl.handle.net/2237/22088 | |||||
識別子タイプ | HDL |