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THREE-STATION OBSERVATIONS OF INTERPLANETARY SCINTILLATION AT 327 MHZ - I
http://hdl.handle.net/2237/22129
http://hdl.handle.net/2237/22129090369eb-0740-48f1-9c3e-b9cf544c6ab9
| 名前 / ファイル | ライセンス | アクション |
|---|---|---|
proria_31_1.pdf (1.7 MB)
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| Item type | 紀要論文 / Departmental Bulletin Paper(1) | |||||
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| 公開日 | 2015-06-01 | |||||
| タイトル | ||||||
| タイトル | THREE-STATION OBSERVATIONS OF INTERPLANETARY SCINTILLATION AT 327 MHZ - I | |||||
| 言語 | en | |||||
| 著者 |
KAKINUMA, Takakiyo
× KAKINUMA, Takakiyo× KOJIMA, Masayoshi |
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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 | Regular observations of interplanetary scintillation at 327MHz have been started with a new three-station system. This paper is a preliminary report of the observations. We have derived the distribution of the solar wind velocity in heliographic latitude and longitude on the solar surface in Mar.-June 1982. In the northern hemisphere, the polar high-speed region with a uniformly high (800 km/s) speed at all latitudes above 45 degrees, such as that observed in 1974-1976, was not yet developed in early 1982. | |||||
| 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 31, p. 1-10, 発行日 1984-03-25 |
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| 著者版フラグ | ||||||
| 値 | publisher | |||||
| URI | ||||||
| 識別子 | http://hdl.handle.net/2237/22129 | |||||
| 識別子タイプ | HDL | |||||
