Possible Tornado-Like Tracks on Mars
- 21 August 1987
- journal article
- other
- Published by American Association for the Advancement of Science (AAAS) in Science
- Vol. 237 (4817) , 883-885
- https://doi.org/10.1126/science.237.4817.883
Abstract
Distinct atmospheric conditions suggest that dark, ephemeral, filamentary lineations on the martian surface may be formed during the passage of intense atmospheric vortices.Keywords
This publication has 13 references indexed in Scilit:
- Dust Devils on MarsScience, 1985
- Measurements of water vapor in Mars' AntarcticIcarus, 1981
- Moderate resolution thermal mapping of Mars: The channel terrain around the Chryse BasinJournal of Geophysical Research, 1979
- Global seasonal variation of water vapor on Mars and the implications for permafrostJournal of Geophysical Research, 1979
- Viking Orbiter imaging observations of dust in the Martian atmosphereJournal of Geophysical Research, 1979
- Frontal systems during passage of the Martian north polar hood over the Viking Lander 2 site prior to the first 1977 dust stormJournal of Geophysical Research, 1979
- Properties and effects of dust particles suspended in the Martian atmosphereJournal of Geophysical Research, 1979
- Mars meteorology: Three seasons at the surfaceGeophysical Research Letters, 1978
- Variable features on Mars. VII. Dark filamentary markings on MarsIcarus, 1976
- Eolian deposits and dunes on MarsJournal of Geophysical Research, 1973