Solar wind plasma entry observed by cluster in the high‐latitude magnetospheric lobes

Using the Cluster data during the period from January to April between 2001 and 2006, we find an observation of solar wind entry due to magnetic reconnection occurred in the terrestrial high‐latitude magnetospheric lobes, tailward of the cusps under northward interplanetary magnetic field (IMF). Occ...

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Veröffentlicht in:	Journal of geophysical research. Space physics 2016-05, Vol.121 (5), p.4135-4144
Hauptverfasser:	Gou, X. C., Shi, Q. Q., Tian, A. M., Sun, W. J., Dunlop, M. W., Fu, S. Y., Zong, Q. G., Facskó, G., Nowada, M., Pu, Z. Y., Mailyan, B., Xiao, T., Shen, X. C.
Format:	Artikel
Sprache:	eng
Schlagworte:	Asymmetry Camber Charged particles Clusters Cusps Interplanetary magnetic field Interplanetary magnetic fields Latitude lobe Lobes Magnetic dipoles Magnetic fields Magnetic reconnection Magnetism Magnetopause Magnetospheres Plasma Skewed distributions Solar magnetic field Solar wind solar wind entry Tilt
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