A magnetic time line for Mars

Details A magnetic time line for Mars A magnetic time line for Mars

Oct 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011epsc.conf..773l&link_type=abstract

EPSC-DPS Joint Meeting 2011, held 2-7 October 2011 in Nantes, France. http://meetings.copernicus.org/epsc-dps2011, p.773

Computer Science

Scientific paper

In this paper, we re-examine the magnetic signature of impact craters as it was measured by MGS. We carefully selected the measurements in order to isolate the spatial variations. We then compare the magnetic field observed directly above these volcanoes or basins to the one measured around them. We conclude that the martian dynamo was most likely active when they were formed, between 3.7 and 3.8 Gyrs ago.

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