The problems of Mars' paleomagnetism

Details The problems of Mars' paleomagnetism The problems of Mars' paleomagnetism

Mar 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988kosis..26..306d&link_type=abstract

Kosmicheskie Issledovaniia (ISSN 0023-4206), vol. 26, Mar.-Apr. 1988, p. 306-314. In Russian.

Computer Science

Dynamo Theory, Mars (Planet), Paleomagnetism, Planetary Magnetic Fields, Deimos, Magnetic Dipoles, Phobos, Terrestrial Planets

Scientific paper

The precession dynamo model suggests that Mars' magnetic field was more intense in the distant past than it is in the present epoch. The orbital parameters of hypothetical Martian satellites, determined from the angular momentum deficit of the present Mars-Phobos-Deimos system, are compared with orbital parameters determined from the precession dynamo model and data on the paleofield of SNC meteorites. It is concluded that the investigation of the paleofields of Mars at the surface and in rock specimens returned to earth is an important way to study the history of the planet, its paleoclimate, and problems of dynamo theory.

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