Stability of the Martian atmosphere: Possible role of heterogeneous chemistry
- 1 March 1990
- journal article
- Published by American Geophysical Union (AGU) in Geophysical Research Letters
- Vol. 17 (3) , 287-290
- https://doi.org/10.1029/gl017i003p00287
Abstract
No abstract availableThis publication has 16 references indexed in Scilit:
- Martian atmosphere studies from the ISM experimentPlanetary and Space Science, 1991
- Solar occultation spectroscopic measurements of the martian atmosphere at 1.9 and 3.7 μmNature, 1989
- Vertical profiles of dust and ozone in the martian atmosphere deduced from solar occultation measurementsNature, 1989
- Diurnal variations in optical depth at MarsIcarus, 1989
- Laboratory studies of sticking coefficients and heterogeneous reactions important in the Antarctic stratosphereGeophysical Research Letters, 1988
- The vertical structure of limb hazes in the Martian atmosphereIcarus, 1986
- Reactions of chlorine nitrate with HCl and H2OGeophysical Research Letters, 1986
- The seasonal and global behavior of water vapor in the Mars atmosphere: Complete global results of the Viking Atmospheric Water Detector ExperimentJournal of Geophysical Research, 1982
- Mariner 9 Television Limb Observations of Dust and Ice Hazes on MarsJournal of the Atmospheric Sciences, 1978
- Photochemistry of the Martian atmosphereIcarus, 1977