Computer Science
Scientific paper
Jan 1989
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989rpsct...2...10d&link_type=abstract
In its JPRS Report: Science and Technology. USSR: Space p 10 (SEE N89-29354 24-12) Transl. into ENGLISH from Kosmicheskiye Issle
Computer Science
Dynamo Theory, Mars (Planet), Paleomagnetism, Planetary Magnetic Fields, Deimos, Magnetic Dipoles, Phobos
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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