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Near-Infrared Spectroscopy of the Surface of Mars Derived from TIGER Spectro-Imaging Data

Published online by Cambridge University Press:  12 April 2016

P. Martin ,
P.C. Pinet ,
R. Bacon  and
A. Rousset
P. Martin
Affiliation:
UPR 234/CNRS, Observatoire Midi-Pyrénées, 31400 Toulouse, France
P.C. Pinet
Affiliation:
UPR 234/CNRS, Observatoire Midi-Pyrénées, 31400 Toulouse, France
R. Bacon
Affiliation:
Observatoire de Lyon, 69561 Saint Genis-Laval Cedex, France
A. Rousset
Affiliation:
Observatoire de Lyon, 69561 Saint Genis-Laval Cedex, France

Abstract

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High spectral and spatial resolution telescopic observations of the western hemisphere of Mars, using the integral field spectrograph TIGER at 0.8-1.1 µm, are described.

Type
3. Integral Field Spectrographs and Spectrometers
Information
International Astronomical Union Colloquium , Volume 149: Tridimensional Optical Spectroscopic Methods in Astrophysics , 1995 , pp. 298 - 299
Copyright
Copyright © Astronomical Society of the Pacific 1995

References

Pinet, P., & Chevrel, S. (1990), J. Geophys. Res., vol. 95, no. B9, 14435.Google Scholar