Variations in Martian surface composition and cloud occurrence determined from thermal infrared spectroscopy: Analysis of Viking and Mariner 9 data
- 25 January 1998
- journal article
- Published by American Geophysical Union (AGU) in Journal of Geophysical Research
- Vol. 103 (E1), 1733-1746
- https://doi.org/10.1029/97je02114
Abstract
No abstract availableThis publication has 45 references indexed in Scilit:
- Hydrous carbonates on Mars?: Evidence from Mariner 6/7 infrared spectrometer and ground‐based telescopic spectraJournal of Geophysical Research, 1994
- Observational evidence of crystalline iron oxides on MarsJournal of Geophysical Research, 1990
- Diurnal variations in optical depth at MarsIcarus, 1989
- The spatial distribution of rocks on marsIcarus, 1986
- Regional dust deposits on Mars: Physical properties, age, and historyJournal of Geophysical Research, 1986
- Martian north polar hazes and surface ice: Results from the Viking Survey/Completion MissionJournal of Geophysical Research: Solid Earth, 1984
- Chemical composition of Martian finesJournal of Geophysical Research, 1982
- Martian dust mantling and surface composition: Interpretation of thermophysical propertiesJournal of Geophysical Research, 1982
- Viking infrared thermal mapperApplied Optics, 1978
- Composition of the Martian dust as derived by infrared spectroscopy from Mariner 9Journal of Geophysical Research, 1975