Buffering of diurnal temperature variations on Venus

Details Buffering of diurnal temperature variations on Venus Buffering of diurnal temperature variations on Venus

Sep 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984icar...59..478j&link_type=abstract

Icarus (ISSN 0019-1035), vol. 59, Sept. 1984, p. 478-480.

Physics

2

Planetary Temperature, Venus (Planet), Atmospheric Temperature, Carbon Dioxide, Degassing, Diurnal Variations, Energy Budgets, Surface Temperature, Venus Atmosphere, Venus, Thermal Properties, Temperature, Diurnal Variations, Outgassing, Calculations, Carbon Dioxide, Calcite, Surface, Energy, Conduction, Insolation, Heating, Atmosphere, Chemical Reactions

Scientific paper

Previous calculations of the role of degassing of CO2 from calcite in buffering the surface temperature of Venus ignored the efficacy with which energy could be conducted into the subsurface. Conduction into the subsurface plays a minor role in the energy balance, however, such that less than 10% of the insolation will conduct into the subsurface and go into degassing CO2, with the remainder heating up the surface and atmosphere; negligible buffering of the surface temperature will occur.

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