A model of the magnetospheric magnetic field

被引：0

作者：

Maltsev, YP ^{[1
]}

Ostapenko, AA ^{[1
]}

机构：

[1] Russian Acad Sci, Kola Sci Ctr, Polar Geophys Inst, Apatity 184200, Murmansk Oblast, Russia

来源：

GEOMAGNETISM AND AERONOMY | 2001年 / 41卷 / 06期

关键词：

D O I：

暂无

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：

An empirical model of the magnetic field at distances of 3 to 40 Earth's radii, depending on the tilt angle of the Earth's dipole, Dst and Kp indices, solar-wind dynamic pressure, and vertical component of the interplanetary magnetic field (IMF) is presented. The magnetic fields are generated by a set of sources, whose position and strength are determined by fitting the magnetic fields observed in experiments. This model is compared with other models.

引用

页码：726 / 731

页数：6

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