Simulation study of near-Earth space disturbances: 1. magnetic storms

被引:5
|
作者
Ebihara, Yusuke [1 ]
机构
[1] Kyoto Univ, Res Inst Sustainable Humanosphere, Uji, Kyoto 6110011, Japan
关键词
Magnetic storms; Computer simulation; Magnetosphere; Ionosphere; Inner magnetosphere; Ring current; PITCH-ANGLE DISTRIBUTIONS; RING CURRENT DEVELOPMENT; SOLAR-WIND CONTROL; PLASMA SHEET; GEOMAGNETIC STORMS; MHD SIMULATIONS; CURRENT PROTONS; NOVEMBER; 2003; MODEL; TIME;
D O I
10.1186/s40645-019-0264-3
中图分类号
P [天文学、地球科学];
学科分类号
07 ;
摘要
A magnetic storm is the world-wide geomagnetic disturbance taking place in near-Earth space environment, lasting for a few days. Geomagnetic fields can be depressed by similar to 1% on the ground for large magnetic storms. The prime cause of the long-lasting, world-wide geomagnetic disturbance is the development of the ring current that surrounds the Earth. The ring current is an electric current carried by charged particles. Thus, the growth and decay of the ring current correspond to accumulation and loss of the ring current particles, respectively. The ring current is strong enough to modulate near-Earth space environment, and leads to many observable effects. In this sense, the ring current can be regarded as an important mediator in the near-Earth space environment. Here, the dynamics and structure of the ring current and its active role are briefly reviewed on the basis of numerical simulation results.
引用
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页数:20
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