A crustal magnetization model for the magnetic field of Mars - A preliminary study of the Tharsis region

Details A crustal magnetization model for the magnetic field of Mars - A preliminary study of the Tharsis region A crustal magnetization model for the magnetic field of Mars - A preliminary study of the Tharsis region

Mar 1997

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1997lpi....28..593h&link_type=abstract

Conference Paper, 28th Annual Lunar and Planetary Science Conference, p. 593.

Physics

Planetary Crusts, Planetary Magnetic Fields, Mars Atmosphere, Meteorites, Magnetic Anomalies

Scientific paper

An initial quantitative investigation is conducted of the hypothesis that a small crustal field whose origin lies in thermal remanent magnetization has existed since that magnetization was acquired during a period of Martian history when a core dynamo field was present. Expected field magnitudes above the Tharsis region, assuming a source region that consists of uniformly magnetized volcamic constructs.

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