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  1. F300 宇宙地球環境研究所
  2. F300b 紀要
  3. Proceedings of the Research Institute of Atmospherics, Nagoya University
  4. 19

VLF HISS OBSERVED AT SYOWA STATION, ANTARCTICA-II : Occurrence and Polarization of VLF Hiss During Disturbances

http://hdl.handle.net/2237/22225
http://hdl.handle.net/2237/22225
f57e2866-214d-42b4-ae27-d06ce01fb9ca
名前 / ファイル ライセンス アクション
proria_19_63.pdf proria_19_63.pdf (4.2 MB)
Item type 紀要論文 / Departmental Bulletin Paper(1)
公開日 2015-06-02
タイトル
タイトル VLF HISS OBSERVED AT SYOWA STATION, ANTARCTICA-II : Occurrence and Polarization of VLF Hiss During Disturbances
言語 en
著者 TANAKA, Yoshihito

× TANAKA, Yoshihito

WEKO 59238

en TANAKA, Yoshihito

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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 The occurrence of VLF hiss is the greatest before the local magnetic midnight. Diurnal variations of occurrence probabilities are remarkably similar in the receiving frequencies of 5, 8, 12, 25 kHz. And they seem to coincide well with the diurnal pattern on the flux intensity of soft electrons (~l kev) precipitating over the station. The maximum energy is received near 10 kHz. There is a positive correlation between the occurrence of VLF hiss and K-index in geomagnetically undisturbed period, but the occurrences decrease during geomagnetic disturbances. The dependence of flux density on geomagnetic activity is also similar to the occurrence of VLF hiss. These facts clearly suggest that VLF hiss is generated in higher altitudes than the auroral ionosphere. The polarization at 12 kHz is independent of geomagnetic activity and the energy of VLF hiss, and it is roughly constant during a discrete VLF event appearing in geomagnetically undisturbed period. These results seem to suggest that wave couplings do not effectively occur in the lower ionosphere and the energy of VLF hiss is decided by the amount of precipitating soft electrons, and that VLF hiss propagates downward in the field aligned duct to an upper region of the auroral ionosphere. The distribution of (R/L) values observed is to be reasonably explained by the simultaneous arrival of multiple waves which independently come down with not so large angles of incidence roughly within the magnetic meridian plane. So, it is concluded that auroral hiss can not propagate to lower latitudes in the earth-ionosphere wave guide because of re-penetration into the auroral ionosphere and the inclination of incident angle toward higher latitude, so that auroral hiss is unique in the auroral zone and it is essentially different from low latitude type VLF hiss.
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 19, p. 63-94, 発行日 1972-03-30
著者版フラグ
値 publisher
URI
識別子 http://hdl.handle.net/2237/22225
識別子タイプ HDL
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