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VLF HISS AT SYOWA STATION, ANTARCTICA
http://hdl.handle.net/2237/22119
http://hdl.handle.net/2237/2211995c6638e-9079-4bd1-b65f-424f9df711cb
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 | VLF HISS AT SYOWA STATION, ANTARCTICA | |||||
言語 | en | |||||
著者 |
TANAKA, Yoshihito
× TANAKA, Yoshihito× NISHINO, Masanori× IWAI, Akira |
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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 | Analyzing the VLF hiss (or auroral hiss) record at Syowa Station (geomagnetic latitude -69.7°) , Antarctica, which induced the observation on polarization, incident angle and intensity, we have found the evidence that VLF hiss is right-handed, and elliptically polarized, wave (whistler mode wave) , and its incident angle into free space below the ionosphere is small. We have also found that the upper frequency of VLF hiss which appear in advance of the break-up of over-head aurora reaches more than 100KHz and that the maximum energy of the spectrum is received at a frequency near to 10 KHz. Further it is suggested that VLF hiss in the auroral zone is generated by Cerenkov radiation process in the low altitude dark magnetosphere, and that it does not propagate to the middle and low latitudes. | |||||
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 17, p. 43-55, 発行日 1970-03-30 |
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著者版フラグ | ||||||
値 | publisher | |||||
URI | ||||||
識別子 | http://hdl.handle.net/2237/22119 | |||||
識別子タイプ | HDL |