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SPECTRUM S-COMPONENT FLUX AND ACTIVE REGION MAGNETIC FIELD
http://hdl.handle.net/2237/22114
http://hdl.handle.net/2237/22114a809041f-f67d-4309-972c-e087376e28ac
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 | 2015-05-29 | |||||
タイトル | ||||||
タイトル | SPECTRUM S-COMPONENT FLUX AND ACTIVE REGION MAGNETIC FIELD | |||||
言語 | en | |||||
著者 |
SHIBASAKI, Kiyoto
× SHIBASAKI, Kiyoto |
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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 | Characteristics are examined of an active region magnetic field structure whose spectral peak of S-component source flux is of a higher frequency than that of normal source. The flux ratio at 3 cm and 8 cm wavelengths (F3/F8) is used as an indicator of peak frequency. The magnetic field structure of an active region with a high flux ratio is compared with a structure with a low flux ratio. It is shown that low-lying magnetic lines of force are characteristic of active regions with high flux ratio. High temperature and high density plasma confined by low-lying magnetic lines of force intensify the flux at short wavelengths, thus the flux peak shift to a shorter wavelength. | |||||
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. 1-9, 発行日 1985-03-25 |
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値 | publisher | |||||
URI | ||||||
識別子 | http://hdl.handle.net/2237/22114 | |||||
識別子タイプ | HDL |