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Influence of Fast Global Variations of Solar Magnetic Fields on Space Weather in Cycle 23
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作者 S. I. Molodykh G. A. Zherebtsov +2 位作者 V. A. Kovalenko j. x. wang V. I. Sidorov 《空间科学学报》 CAS CSCD 北大核心 2005年第5期460-467,共8页
It is established that the large-scale and global magnetic fields in the Sun's atmosphere do not change smoothly, and long-lasting periods of gradual variations are superseded by fast structural changes of the glo... It is established that the large-scale and global magnetic fields in the Sun's atmosphere do not change smoothly, and long-lasting periods of gradual variations are superseded by fast structural changes of the global magnetic field. Periods of fast global changes on the Sun are accompanied by anomalous manifestations in the interplanetary space and in the geomagnetic field. There is a regular recurrence of these periods in each cycle of solar activity, and the periods are characterized by enhanced flaring activity that reflects fast changes in magnetic structures. Is demonstrated, that the fast changes have essential influencing on a condition of space weather, as most strong geophysical disturbances are connected to sporadic phenomena on the Sun. An explanation has been offered for the origin of anomalous geomagnetic disturbances that are unidentifiable in traditionally used solar activity indices. Is shown, main physical mechanism that leads to fast variations of the magnetic fields in the Sun's atmosphere is the reconnection process. 展开更多
关键词 太阳活动 磁场 空间气候 大气 动态变化 太阳光
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