| 行星际起伏场通过激波后的变化 |
| |
| 引用本文： | 魏奉思.行星际起伏场通过激波后的变化[J].空间科学学报,1983,3(3):184-194. |
| |
| 作者姓名： | 魏奉思 |
| |
| 作者单位： | 中国科学院空间物理研究所 |
| |
| 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。
|
| 收稿时间： | 1982-11-23 |
THE VARIATIONS OF THE INTERPLANETARY FLUCTUATIONS ACROSS THE SHOCK WAVE |
| |
| Institution: | Institute of Space Physics, Aeademia Sinica |
| |
| 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. |
| |
| Keywords: | |
| 本文献已被 CNKI 等数据库收录！ |
| 点击此处可从《空间科学学报》浏览原始摘要信息 |
| 点击此处可从《空间科学学报》下载免费的PDF全文 |
