Transformation of solar wind energy into the energy of magnetospheric processes

被引:0
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作者
P. A. Sedykh
机构
[1] Siberian Branch of Russian Academy of Sciences,ISTP
来源
关键词
Solar wind-geomagnetosphere interaction; Bow shock; Magnetosheath; Poynting flux; Collisionless plasma;
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摘要
When the solar wind flows round the magnetosphere, its flow structure and interplanetary magnetic field lines are affected. This indicates the appearance of an electric current system in near-Earth space. the magnetized solar wind plasma moving at the solar wind velocity in the coordinate system of near-earth bow shock induces an electric field in this system. When crossing the bow shock front at the nose point, the tangential magnetic field component increases nearly four times, and the magnetic field energy density—15 times.
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页码:1 / 15
页数:14
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