Some diurnal properties of clouds over the Martian volcanoes

Details Some diurnal properties of clouds over the Martian volcanoes Some diurnal properties of clouds over the Martian volcanoes

Jul 1980

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980natur.286..362h&link_type=abstract

Nature, vol. 286, July 24, 1980, p. 362-364. Research supported by the Science Research Council and NASA.

Computer Science

5

Clouds (Meteorology), Mars Atmosphere, Diurnal Variations, Ice Clouds, Mars Craters, Mars Photographs, Topography, Viking Orbiter Spacecraft, Volcanoes, Mars, Clouds, Volcanoes, Thermal Properties, Diurnal Variations, Dust, Seasons, Ascraeus Mons, Elysium Mons, Atmosphere, Storms, Observations, Meteorology, Viking Orbiters, Water Vapor, Thermodynamics, Cycles, Photographs, Analysis, Topography, Composition, Cooling, Heating, Circulation, Formation, Winds

Scientific paper

The diurnal properties of cloud systems over Martian volcanoes observed by the Viking Orbiter spacecraft are discussed. Photographic sequences of diurnal cloud development are presented for clouds in the vicinity of Elysium Mons and Ascraeus Mons, and the rapid growth of cloudiness starting at 11.23 LT is noted. The low-lying fogs and convective afternoon clouds observed are characterized as water ice clouds, while the cirrus-type clouds may be composed of CO2. The diurnal development of the clouds is then explained in terms of local atmospheric stability and circulation as influenced by surface topography and thermal properties. Consideration is also given to possible reasons for the pronounced seasonal variations in cloudiness.

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