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- W2028321912 abstract "view Abstract Citations (10) References (5) Co-Reads Similar Papers Volume Content Graphics Metrics Export Citation NASA/ADS Blue Haze and the Vertical Structure of the Martian Atmosphere. Hess, Seymour L. Abstract The atmospheric haze which usually obscures the surface of Mars in blue light is probably a condensate rather than a dust because it can clear away rapidly. Carbon dioxide and water vapor are both present in the atmosphere, and condensation of each into the solid phase has been suggested to explain the blue haze. Calculations are carried out by assuming a convective atmosphere with a surface temperature of +10 C for the subsolar point and a lapse rate of 3.7 C/km. When the optical properties of clouds produced in such an atmosphere are determined with the aid of the Mie theory of scattering, it is found that (1) carbon dioxide ice clouds are far too opaque to be the cause of the blue haze; (2) water ice clouds can cause the blue haze if the surface frost point lies near -90 C. The second result is consistent with the failure of all modern attempts to detect water vapor spectroscopically in the Martian atmosphere, since the total precipitable water content corresponding to such a frost point is only 2 These results indicate that the author's earlier suggestion of carbon dioxide ice clouds should be rejected. Publication: The Astrophysical Journal Pub Date: May 1958 DOI: 10.1086/146504 Bibcode: 1958ApJ...127..743H full text sources ADS |" @default.
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- W2028321912 date "1958-05-01" @default.
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- W2028321912 title "Blue Haze and the Vertical Structure of the Martian Atmosphere." @default.
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