Oct 1982
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982esasp.185...29f&link_type=abstract
In ESA The Planet Mars p 29-36 (SEE N83-19673 09-91)
Physics
Dust Storms, Energy Budgets, Mars (Planet), Planetary Atmospheres, Planetary Ionospheres, European Space Programs, Gravitational Fields, Interplanetary Spacecraft, Mars Surface, Planetary Magnetospheres, Solar Wind, Topography, Water Vapor
Scientific paper
The Martian atmospheric and ionospheric structure, time behavior and chemical composition; its global energy budget and thermal evolution in particular during dust storms are discussed. The content of water vapor and its time variation, the gravity field, and topography of the planet, the Martian intrinsic magnetic field, and the solar wind interaction with Mars (magnetospheric versus ionospheric) are addressed in terms of the objective of the geophysical orbiter KEPLER.
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