Preliminary Analysis of Microwave Brightness Temperature of the Lunar Surface from Chang-E 1 Multi-Channel Radiometer Observation and Inversion of Regolith Layer Thickness

Details Preliminary Analysis of Microwave Brightness Temperature of the Lunar Surface from Chang-E 1 Multi-Channel Radiometer Observation and Inversion of Regolith Layer Thickness Preliminary Analysis of Microwave Brightness Temperature of the Lunar Surface from Chang-E 1 Multi-Channel Radiometer Observation and Inversion of Regolith Layer Thickness

Mar 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010lpi....41.1331j&link_type=abstract

41st Lunar and Planetary Science Conference, held March 1-5, 2010 in The Woodlands, Texas. LPI Contribution No. 1533, p.1331

Physics

Scientific paper

Using Chang-E 1 microwave radiometer observation, a global regolith
thickness map was inverted and the global abundance of 3He in the
regolith was estimated.

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