Lunar Titanium Characterization Based on Chang'E (CE-1) Interference Imaging Spectrometer (IIM) Imagery and RELAB Spectra

Details Lunar Titanium Characterization Based on Chang'E (CE-1) Interference Imaging Spectrometer (IIM) Imagery and RELAB Spectra Lunar Titanium Characterization Based on Chang'E (CE-1) Interference Imaging Spectrometer (IIM) Imagery and RELAB Spectra

Mar 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010lpi....41.1642l&link_type=abstract

41st Lunar and Planetary Science Conference, held March 1-5, 2010 in The Woodlands, Texas. LPI Contribution No. 1533, p.1642

Physics

Scientific paper

FWHM, absorption position, absorption depth, absorption area and
absorption asymmetry are used to characterize titanium spectral features
by Chang’E-1 and RELAB data around Apollo 17 and 16 landing sites.

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