Hostname: page-component-cd9895bd7-hc48f Total loading time: 0 Render date: 2024-12-26T04:58:17.340Z Has data issue: false hasContentIssue false
  • English
  • Français

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

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

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