Imaging and spectroscopy of Mars from 1.56 to 4.16 um: 1994-95 IRTF observations

Jim Bell, Cornell University

Co-authors: Bill Golisch, Dave Griep, Charlie Kaminski (NASA/IRTF); Ted Roush (SFSU/NASA Ames); Dave Klassen (U. Wyoming)

  • Viewgraphs

    SLIDES: 

      SLIDE     DESCRIPTION
    

    
 dps95_01 3 micron band depth map vs. topography
    
 dps95_02 4.1 micron (atmospheric) band depth vs. topography
    
 dps95_03 3.8 micron band depth vs. topography
    
 dps95_04 3.776 micron albedo vs. Viking-derived (1977) albedo
    
 dps95_05 3.776 micron albedo vs. HST 1.042 micron image (1995)
    
 dps95_06 3.0 micron band depth vs. 3.776 micron albedo
    
 dps95_07 4.106 micron (surface?) band depth vs. topography
    
 dps95_08 3.32 and 3.40 micron band vs. albedo and topography
    
 dps95_09 3.32 micron band depth vs albedo, at two different times
    
 dps95_10 3.40 micron band depth vs albedo, at two different times
    
 dps95_11 Grid of many wavelength obtained on 4 February 1995

    Last Modified by Jim Bell on 8 November 1995.
    Mail to: jimbo@cuspif.tn.cornell.edu