摘要
In previous studies, the magnetic field structures in the solar wind and in the magnetosheath usually have a high dependence on only the Y component. In this study, we compared the simultaneous data from OMNI database, THEMIS-B in the solar wind, and THEMIS-C in the magnetosheath to investigate the relationship between the magnetic field structures in the solar wind and in the magnetosheath under the radial IMF conditions. We find that B z has a better correlation than B y between the magnetic fields in the two regions, and the correlation for B x is poor. When the magnetic field transits through the bow shock, the magnetic field will be enhanced in all components, especially in B y . After that, B x will divert to the Y and Z components, but the diversion to B y will be larger than that to B z in this case.
原文 | ???core.languages.en_GB??? |
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頁(從 - 到) | 181-187 |
頁數 | 7 |
期刊 | Advances in Space Research |
卷 | 58 |
發行號 | 2 |
DOIs | |
出版狀態 | 已出版 - 15 7月 2016 |