Subsurface Magnetized Source Layers Underneath the Mare Crisium Observed by Lunar Radar Sounder

Details Subsurface Magnetized Source Layers Underneath the Mare Crisium Observed by Lunar Radar Sounder Subsurface Magnetized Source Layers Underneath the Mare Crisium Observed by Lunar Radar Sounder

Mar 2012

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2012lpi....43.1380b&link_type=abstract

43rd Lunar and Planetary Science Conference, held March 19–23, 2012 at The Woodlands, Texas. LPI Contribution No. 1659, id.1380

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Scientific paper

We evaluated subsurface stratification and its thickness as magnetized
source layers by using Lunar Radar Sounder data. Our results imply lunar
core dynamo had been driven at least during 3.47 Ga to 3.67 Ga.

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