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| Titel |
Solar Wind Entry into The High-Latitude Magnetospheric lobes: Cluster Observations |
| VerfasserIn |
Xiaochen Gou, Quanqi Shi |
| Konferenz |
EGU General Assembly 2014
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| Medientyp |
Artikel
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| Sprache |
Englisch
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| Digitales Dokument |
PDF |
| Erschienen |
In: GRA - Volume 16 (2014) |
| Datensatznummer |
250097607
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| Publikation (Nr.) |
 EGU/EGU2014-16989.pdf |
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| Zusammenfassung |
| During the quiet times when the interplanetary magnetic field (IMF) is northward, using Cluster multi-spacecrafts observation data between August to October each year from 2002 to 2004, Shi, et al. [2013] reported an unexpected discovery observation of regions of solar wind entry into the Earth’s high-latitude magnetosphere tailward of the cusps where the solar wind plasmas may penetrate into magnetosphere through the mechanism of high-latitude magnetic reconnection. Through From statistical analysis, they fouind that the IMF Bx component may influence the solar wind entry into the magnetosphere by changing the occurring conditions of high-latitude magnetic reconnection. Based on their studies, in this paper we used another period Cluster data which is between January to April each year from 2001 to 2006 to do a some further study, . as As a result, the influence of the IMF Bx component is consistent with the results from Shi, et al. [2013].In addition, wWe also found find that the IMF By component influenced affects the events changed withalong with the IMF Bx component, which is conform consistent withto the Parker Spiral of the IMF. |
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