A Martian Paleomagnetic Pole Estimate Made Using the Distribution and Intensity of Large Scale Magnetic Features

Details A Martian Paleomagnetic Pole Estimate Made Using the Distribution and Intensity of Large Scale Magnetic Features A Martian Paleomagnetic Pole Estimate Made Using the Distribution and Intensity of Large Scale Magnetic Features

Mar 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005lpi....36.1720p&link_type=abstract

36th Annual Lunar and Planetary Science Conference, March 14-18, 2005, in League City, Texas, abstract no.1720

Physics

Scientific paper

Using the the regional distribution of magnetization, we deduce a new
paleomagnetic pole associated with the large magnetic features of the
Cimmeria region. The pole would suggest that the Tharsis bulge was
within 20 degrees of the magnetic equator when the Martian magnetic
field was active.

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