The opacity of some local Martian dust storms observed by the Viking IRTM
- 31 March 1980
- Vol. 41 (3) , 389-399
- https://doi.org/10.1016/0019-1035(80)90223-7
Abstract
No abstract availableKeywords
This publication has 10 references indexed in Scilit:
- Thermal infrared properties of the Martian atmosphere: 4. Predictions of the presence of dust and ice clouds from Viking IRTM spectral measurementsJournal of Geophysical Research, 1979
- Thermal infrared properties of the Martian atmosphere: 3. Local dust cloudsJournal of Geophysical Research, 1979
- Thermal infrared properties of the Martian atmosphere: 1. Global behavior at 7, 9, 11, and 20 μmJournal of Geophysical Research, 1979
- Viking Orbiter imaging observations of dust in the Martian atmosphereJournal of Geophysical Research, 1979
- Thermal tides and Martian dust storms: Direct evidence for couplingJournal of Geophysical Research, 1979
- Properties and effects of dust particles suspended in the Martian atmosphereJournal of Geophysical Research, 1979
- On the opacity of Martian dust storms derived by Viking IRTM spectral measurementsJournal of Geophysical Research, 1979
- Thermal and albedo mapping of Mars during the Viking primary missionJournal of Geophysical Research, 1977
- Properties of aerosols in the Martian atmosphere, as inferred from Viking Lander imaging dataJournal of Geophysical Research, 1977
- Physical properties of the particles composing the Martian dust storm of 1971–1972Icarus, 1977