Clementine 2.7 µm Data and 70-cm Earth-based Radar Data Provide Additional Constraints for UVVIS-based Estimates of TiO2 Content for Lunar Mare Basalts

Details Clementine 2.7 µm Data and 70-cm Earth-based Radar Data Provide Additional Constraints for UVVIS-based Estimates of TiO2 Content for Lunar Mare Basalts Clementine 2.7 µm Data and 70-cm Earth-based Radar Data Provide Additional Constraints for UVVIS-based Estimates of TiO2 Content for Lunar Mare Basalts

Mar 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005lpi....36.2254g&link_type=abstract

36th Annual Lunar and Planetary Science Conference, March 14-18, 2005, in League City, Texas, abstract no.2254

Computer Science

2

Scientific paper

Looking to improve the accuracy of your UVVIS derived TiO2 compositions
for lunar basalts? Look no further, 2.7 micron and 70-cm radar data sets
provide complementary information to the UVVIS ratio that may improve
your estimates of TiO2 composition.

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