Mapping Homogeneous Mare Basalt Units in the Aristarchus Quadrangle Using Clementine Spectral Parameters

Details Mapping Homogeneous Mare Basalt Units in the Aristarchus Quadrangle Using Clementine Spectral Parameters Mapping Homogeneous Mare Basalt Units in the Aristarchus Quadrangle Using Clementine Spectral Parameters

Mar 2012

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2012lpi....43.1133z&link_type=abstract

43rd Lunar and Planetary Science Conference, held March 19–23, 2012 at The Woodlands, Texas. LPI Contribution No. 1659, id.1133

Computer Science

Scientific paper

In our work, multi-dimensional spatial distribution of several
Clementine spectral parameters was used to identify and determine basalt
units, which related to the composition of the lunar interior and its
thermal evolution.

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