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- W2029382303 startingPage "3213" @default.
- W2029382303 abstract "Selected surface temperatures, consistent with the Mariner 4 observations, are used to calculate the radiative heat budget and radiative equilibrium temperature distributions of the atmosphere of Mars as a function of latitude for the summer season. The results indicate that below about 40° latitude there is a surplus of radiational energy and that above 40° latitude there is a deficit. For balance to prevail, there must exist a transport of energy across the 40° latitude of about 1016 cal min−1. Radiative cooling due to the 15-μ band of CO2 predominates at all levels and latitudes except at a height of about 7.5 km and is about an order of magnitude greater than the heating due to incoming solar radiation. The radiative equilibrium temperature distribution indicates an isothermal layer above about 60 km, but this region is not well defined." @default.
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- W2029382303 date "1968-05-15" @default.
- W2029382303 modified "2023-09-26" @default.
- W2029382303 title "Radiative equilibrium temperature distribution of the atmosphere of Mars" @default.
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- W2029382303 doi "https://doi.org/10.1029/jb073i010p03213" @default.
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