Dynamics of the Earth's Outer Radiation Belt in November 2009 Based on the Experimental Data from the CORONAS-Photon and Meteor-M No. 1 Satellites

被引:3
|
作者
Barinova, V. O. [1 ]
Bogomolov, A. V. [1 ]
Kalegaev, V. V. [1 ]
Myagkova, I. N. [1 ]
Panasyuk, M. I. [1 ]
Parunakyan, D. A. [1 ]
Rubinshtein, I. A. [1 ]
Ryazantseva, M. O. [1 ]
Starostin, L. I. [1 ]
机构
[1] Moscow MV Lomonosov State Univ, Skobeltsyn Inst Nucl Phys, Moscow 119991, Russia
基金
俄罗斯基础研究基金会;
关键词
electrons; Earth's radiation belt; solar wind; RELATIVISTIC ELECTRONS; ENERGETIC ELECTRONS; MAGNETIC STORMS; MAGNETOSPHERE; ACCELERATION; SCATTERING; DIFFUSION; WAVES;
D O I
10.3103/S0027134911060038
中图分类号
O4 [物理学];
学科分类号
0702 ;
摘要
The dynamics of the Earth's outer radiation belt were traced at altitudes of 500-830 km during weak geomagnetic disturbances based on the data of simultaneous experiments carried out in November 2009 onboard the CORONAS-Photon solar observatory and the Meteor-M No. 1 artificial satellite. The average statistical profile of external boundary of the outer radiation belt that is characteristic for a quiet magneto-sphere has been found from the analysis of variations in the position of the polar boundary of the capture region in the Earth's magnetosphere.
引用
收藏
页码:616 / 621
页数:6
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