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• W1982176724 startingPage "719" @default.
• W1982176724 abstract "The global density distribution of atomic H in the upper atmosphere of Venus is determined in terms of a global circulation model. It is shown that H produced on the dayside is efficiently advected to the nightside by the major gas CO2 where it is then convected to lower altitudes and recombines. A maximum night/day H density ratio of about 5 is derived, in which case exospheric return flow from night to day strongly limits the nightside density enhancement. A previously postulated constraint connecting the eddy diffusion coefficient with the escape flux of H in one dimensional models is no longer required when global circulation of H is considered." @default.
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• W1982176724 date "1978-08-01" @default.
• W1982176724 modified "2023-10-16" @default.
• W1982176724 title "Global circulation and distribution of hydrogen in thermosphere of Venus" @default.
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• W1982176724 doi "https://doi.org/10.1029/gl005i008p00719" @default.
• W1982176724 hasPublicationYear "1978" @default.
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