Computer Science
Scientific paper
Feb 1991
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991icar...89..377l&link_type=abstract
Icarus (ISSN 0019-1035), vol. 89, Feb. 1991, p. 377-383.
Computer Science
16
Atmospheric Chemistry, Atmospheric Models, Jupiter Atmosphere, Photochemical Reactions, Stratosphere, Troposphere, Abundance, Atmospheric Composition, Carbon Monoxide, Ethane, Mixing Height, Tropopause, Juputer, Atmosphere, Troposphere, Stratosphere, Photochemistry, Models, Calculations, Concentration, Flux, Flow, Mixing, Eddy Diffusion, Numerical Methods, Simulations, Carbon Monoxide, Ethane, Abundance, Tropopause
Scientific paper
The case of a chemically unreactive species flowing downward through the stratosphere and troposphere with a constant flux is presently treated by a one-dimensional Jovian atmosphere model which encompasses the coupling between a rapidly mixed troposphere and a stagnant stratosphere, so that the contrast between the peak stratosphere and tropopause concentrations is reflective of the variation between the lower stratosphere and upper troposphere eddy diffusion coefficients. Numerical simulations of unreactive CO and C2H6 species indicate that upper troposphere abundances may possess a substantial photochemical contribution. The implications of these modeling results for higher spectral resolution observations are noted.
Allen Marsha M.
Landry B.
Yung Yuk L.
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