The Microwave Anomalies of the Lunar Far-Side and South Pole — The Chang'E-1 Microwave Sounder (CELMS) Results

Details The Microwave Anomalies of the Lunar Far-Side and South Pole — The Chang'E-1 Microwave Sounder (CELMS) Results The Microwave Anomalies of the Lunar Far-Side and South Pole — The Chang'E-1 Microwave Sounder (CELMS) Results

Mar 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010lpi....41.1176j&link_type=abstract

41st Lunar and Planetary Science Conference, held March 1-5, 2010 in The Woodlands, Texas. LPI Contribution No. 1533, p.1176

Physics

Scientific paper

CELMS shows the farside TBL is lower than the nearside, while the
regolith thickness is thicker. The dielectric constant in the area
40S-70S, 159W-150E is fairly low. CELMS shows that it cannot rule out
the possibility of water existing at the lunar pole.

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