Upstream Proton Cyclotron Waves at Mars During the Passage of ICMEs

The presence of proton cyclotron waves (PCWs) upstream from Mars indicates picked up protons originating from the Martian extended hydrogen (H) exosphere by the solar wind and loss of H to interplanetary space. The occurrences and properties of PCWs associated with normal solar wind conditions have...

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Veröffentlicht in:	Journal of Geophysical Research: Planets 2023-05, Vol.128 (5), p.n/a
Hauptverfasser:	Zhao, Dan, Guo, Jianpeng, Lin, Haibo, Mazelle, Christian, He, Linxia, Meng, Weiduo, Chen, Yan, Kong, LingGao, Wei, Yong, Liu, Libo
Format:	Artikel
Sprache:	eng
Schlagworte:	Coronal mass ejection Cyclotrons Ellipticity Exosphere Extreme weather Hydrogen Interplanetary space Magnetic fields Mars Mars atmosphere Mars environment Perihelions Protons Sciences of the Universe Solar wind Space weather Spacecraft Upstream Wave propagation Weather Weather conditions
Online-Zugang:	Volltext
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