VLF-Noise in the Dayside Polar Cusp
スポンサーリンク
概要
- 論文の詳細を見る
VLF-noise measurements at several Antarctic ground stations (Mirny, Sleightrain and Vostok) are used as diagnostic of the parameters of the solar wind particles penetrating in the polar cusp region. The observed results revealed the higher level radiation zone in the dayside polar cusp region (geomagnetic latitude ∿79°) when Kp≤3; two maxima of the daily intensity of VLF noise occur around 12 h and 18 h (local magnetic time). The coincidence in time of the VLF noise growth with soft electrons precipitation probability maxima indicates that VLF noise in the dayside polar cusp is generated by precipitating soft electrons.
- 国立極地研究所の論文
著者
-
Kleimenova N.g.
Institute Of Physics Of The Earth Academy Of Sciences Of The Ussr
-
Golikov Yu.V.
Institute of Physics of the Earth,Academy of Sciences of the USSR
-
Troitskaya V.A.
Institute of Physics of the Earth,Academy of Sciences of the USSR
-
Golikov Yu.v.
Institute Of Physics Of The Earth Academy Of Sciences Of The Ussr
-
Troitskaya V.a.
Institute Of Physics Of The Earth Academy Of Sciences Of The Ussr
関連論文
- Equatorial enhancement of Pc5-6 magnetic storm tme geomagnetic pulsations
- VLF-Noise in the Dayside Polar Cusp