Intensity of Pc5 Geomagnetic Pulsations Observed on the Earth's Surface, Depending on the Corresponding Oscillation Mode (Poloidal or Toroidal) in the Magnetosphere

被引:1
|
作者
Roldugin, V. K. [1 ]
机构
[1] Russian Acad Sci, Kola Sci Ctr, Apatity Div, Polar Geophys Inst, Apatity 184209, Murmansk Oblast, Russia
基金
俄罗斯基础研究基金会;
关键词
ULF WAVES; RELATIVISTIC ELECTRONS; COMPREHENSIVE SURVEY; ALFVEN WAVES; CLUSTER;
D O I
10.1134/S001679321302014X
中图分类号
P3 [地球物理学]; P59 [地球化学];
学科分类号
0708 ; 070902 ;
摘要
Thirty-six cases of Pc5 geomagnetic pulsations on the GOES-8 geostationary satellite for 2001, which had amplitudes equal to several nanoteslas and continued for more than an hour, have been studied. Twenty-two and 14 pulsations were toroidal and poloidal, respectively. All these pulsations were compared with geomagnetic observations at the Poste-de-la-Baleine observatory (PBQ), which was located near the satellite projection. It was established that the pulsation frequencies on the ground and in the magnetosphere do not always coincide. It has been detected that poloidal oscillations have small and large amplitudes on the ground and in the magnetosphere, respectively; the situation is opposite for toroidal oscillations. The amplitude of ground-level pulsations to a larger degree depends on the azimuthal field component in the magnetosphere than on the radial component.
引用
收藏
页码:157 / 165
页数:9
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