Physics
Scientist
Laboratory for Atmospheric and Space Physics, University of Colorado, Boulder, Colorado 80303, USA
Laboratory for Atmospheric and Space Physics, University of Colorado, Boulder, CO 80303, USA
University of Colorado, USA
Laboratory for Atmosphere and Space Physics, Boulder, CO, USA;
Laboratory for Atmosphere and Space Physics, University of Colorado, Boulder, CO, USA;
LASP, University of Colorado, Boulder, CO, USA;
University of Colorado / Laboratory for Atmospheric and Space Physics, 1234 Innovation Drive, Boulder, CO 80303
Laboratory for Atmospheric and Space Physics, University of Colorado, Boulder, CO, USA
University of Colorado, Laboratory for Atmospheric and Space Physics 1234 Innovation Drive, Boulder, CO 80303, USA gregory.
University of Colorado, Laboratory for Atmospheric and Space Physics, 1234 Innovation Dr, Boulder, CO 80303
Laboratory for Atmospheric and Space Physics, University of Colorado, Boulder, CO 80303, USA for Atmospheric and Space Physics, Univ. Colo., Boulder, Boulder, CO 80303
University of Colorado, Laboratory for Atmospheric and Space Physics, 1234 Innovation Dr, Boulder, CO 80303, USA
Laboratory for Atmospheric and Space Physics, University of Colorado, 1234 Innovation Drive, Boulder, CO 80303, USA
JPL, Caltech, Pasadena, CA, USA
LASP, University of Colorado, Boulder, CO, USA
Laboratory for Atmospheric and Space Physics, University of Colorado, Boulder, CO, USA for Atmospheric and Space Physics, University of Colorado, Boulder, CA, USA
A comparison of the ultraviolet to near-infrared spectral properties of Mercury and the Moon as observed by MESSENGER
An Overview of Ultraviolet Through Infrared Reflectance Observations of Mercury during the Second Messenger Flyby.
An Overview of Ultraviolet Through Infrared Reflectance Spectroscopic Observations of Mercury During the First MESSENGER Flyby
Analysis of Surface Reflectance Spectroscopy From the First MESSENGER Flyby of Mercury
Analysis of the Dedicated Spectral Photometric Observations from MESSENGER's Third Mercury Flyby
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