THE VARIATIONS OF THE INTERPLANETARY FLUCTUATIONS ACROSS THE SHOCK WAVE
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摘要: 本文采用磁流体平面斜激波模型探讨了行星际起伏场(包括磁场和等离子体速度)通过激波后的变化。得到的近似解析解表明:由本模型所得到的结果能较好地解释人们[1,2]对行星际、磁鞘层观测资料进行统计研究所得到的认识。Abstract: The variations of the interplanetary fluctuations across the shock wave are discussed on the basis of the theory of MHDshock wave.The approximate analysis solution shows that our theoretical results can explain better the statistic results obtained by Belcher and Davis (1971) and Whang (1973) who analysed observation data from Mariner 5 and Explorer 34 in the interplanetary space and the magnetosheath.
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