Induced Magnetic Fields and Plasma Motions in the Inner Part of the Martian Magnetosphere

Analysis of Mars Atmosphere and Volatile Evolution (MAVEN)/Supra‐Thermal And Thermal Ion Composition observations in the Martian upper atmosphere, bounded at higher altitudes by the shocked solar wind, shows that the draping of interplanetary magnetic field penetrates down to low altitudes (∼200−250...

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Veröffentlicht in:	Journal of geophysical research. Space physics 2021-12, Vol.126 (12), p.n/a
Hauptverfasser:	Dubinin, E., Fraenz, M., Modolo, R., Pätzold, M., Tellmann, S., Vaisberg, O., Shuvalov, S., Zelenyi, L., Chai, L., Wei, Y., McFadden, J., DiBraccio, G., Espley, J.
Format:	Artikel
Sprache:	eng
Schlagworte:	Asymmetry Coordinate systems Coordinates Electric fields Hemispheres IMF Interplanetary magnetic field Ion acceleration Ion composition Ion dynamics Ion extraction Ionosphere Ionospheric plasma Low altitude Magnetic fields Magnetic properties Magnetism Magnetosheath magnetosphere Mars Mars atmosphere Mars ionosphere Mars missions Mars spacecraft Physics Planetary ionospheres Planetary magnetic fields Planetary magnetospheres Plasma Plasma Physics Recoil reconnection Sciences of the Universe Solar wind Spacecraft Upper atmosphere
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