Vertical profiles of dust and ozone in the Martian atmosphere deduced from solar occultation measurements
- 28 February 1991
- journal article
- Published by Elsevier in Planetary and Space Science
- Vol. 39 (1-2) , 175-187
- https://doi.org/10.1016/0032-0633(91)90140-6
Abstract
No abstract availableKeywords
This publication has 12 references indexed in Scilit:
- Mapping of CO millimeter-wave lines in Mars' atmosphere: The spatial variability of carbon monoxide on MarsPlanetary and Space Science, 1991
- Ice haze, snow, and the Mars water cycleJournal of Geophysical Research, 1990
- 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
- Results from the ISM experimentNature, 1989
- The vertical structure of limb hazes in the Martian atmosphereIcarus, 1986
- Spectroscopy of molecular oxygen in the Atmospheres of Venus and MarsIcarus, 1983
- The Mariner 5 Ultraviolet Photometer Experiment: Analysis of hydrogen lyman alpha dataJournal of Geophysical Research, 1976
- Light scattering in planetary atmospheresSpace Science Reviews, 1974
- Limb-darkening observations between 1800 and 2900 ÅSolar Physics, 1968