Observation of Plasma Instability on the Dayside Region between Magnetosheath and Ionosphere of Mars

The interaction of the solar wind with the plasma envelope of planets without their own global magnetic field has a different character than does the corresponding process near the Earth due to the closer location of the bow shock to the planet’s surface. Similar processes and structures in the inte...

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Veröffentlicht in:	Cosmic research 2021-11, Vol.59 (6), p.493-500
Hauptverfasser:	Kim, K. I., Shuvalov, S. D.
Format:	Artikel
Sprache:	eng
Schlagworte:	Astronomy Astrophysics and Astroparticles Astrophysics and Cosmology Electric fields Instability Ionosphere Kelvin-Helmholtz instability Magnetic fields Magnetohydrodynamic stability Magnetosheath Mars Mars atmosphere Mars ionosphere Mars missions Mars spacecraft Physics Physics and Astronomy Planetary ionospheres Planetary magnetospheres Planets Plasma Plasma instabilities Solar wind Space Exploration and Astronautics Space Sciences (including Extraterrestrial Physics Spacecraft Stability analysis Velocity Vortices
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