Other
Scientific paper
Jan 1997
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1997adspr..20..155v&link_type=abstract
Advances in Space Research, vol. 20, p. 155
Other
5
Mars Atmosphere, Bow Waves, Shock Wave Propagation, Planetary Magnetospheres, Plasma Dynamics, Satellite Observation, Self Consistent Fields, Shock Wave Profiles, Magnetopause
Scientific paper
The Mars planetary bow shock motion and its shape variation under the
influence of variations of the external plasma flow parameters and the
shape of the magnetopause are here described by a self-consistent
quantitative model. The model is applicable to other planetary bow
shocks, including those with unusually low Mach numbers.
Kotova Galina A.
Remizov A. P.
Riedler Willi
Rosenbauer Helmut
Schwingenschuh Konrad
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