Effects of Solar Wind Density and Velocity Variations on the Martian Ionosphere and Plasma transport—A MHD Model Study

Solar wind dynamic pressure, consisting solar wind density nsw and velocity Vsw, is an important external driver that controls Martian plasma environment. In this study, a 3D magnetohydrodynamic model is applied to investigate the separate influences of solar wind density and velocity on the Martian...

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Veröffentlicht in:	Journal of geophysical research. Space physics 2023-12, Vol.128 (12), p.n/a
Hauptverfasser:	Song, Yihui, Lu, Haoyu, Cao, Jinbin, Wu, Xiaoshu, Liu, Yang, Li, Shibang, Wang, Siqi, Wild, James A., Zhou, Chenling, Wang, Jianxuan, Chen, Nihan
Format:	Artikel
Sprache:	eng
Schlagworte:	Aerospace environments crustal field Density Dynamic pressure Flow distribution Flow pattern Hall MHD simulation Ion transport Ion velocity Ionosphere Ions Magnetic fields Magnetic shielding Magnetohydrodynamics Mars Mars atmosphere Mars ionosphere Martian ionosphere Night Outflow Planetary ionospheres Planetary magnetic fields Plasma plasma transport Solar wind Solar wind density solar wind dynamics pressure Solar wind effects Solar wind particles Solar wind velocity Southern Hemisphere Spatial distribution Three dimensional models Transport processes Velocity Water outflow Wind effects Wind speed Wind velocities
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