Phosphine photochemistry in the atmosphere of Saturn

Details Phosphine photochemistry in the atmosphere of Saturn Phosphine photochemistry in the atmosphere of Saturn

Sep 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984icar...59..314k&link_type=abstract

Icarus (ISSN 0019-1035), vol. 59, Sept. 1984, p. 314-335. NASA-supported research.

Computer Science

30

Atmospheric Chemistry, Phosphines, Photochemical Reactions, Saturn Atmosphere, Atmospheric Models, Concentration (Composition), Reaction Kinetics, Turbulent Diffusion, Saturn, Phosphine, Photochemistry, Atmosphere, Models, Troposphere, Stratosphere, Ammonia, Hydrocarbons, Altitude, Tropopause, Eddies, Sublimation, Formations, Chemical Reactions, Density, Gases, Data, Phases, Organic Compounds, Production Rates, Diffusion, Temperature, Concentration, Minor Elements, Parameters

Scientific paper

The photochemistry of PH3 in the atmosphere of Saturn is studied, including the effects of coupling with the photochemistries of NH3 and hydrocarbons. The vertical concentration of PH3 is found to be extremely sensitive to the eddy diffusion coefficient (K) profile used. If K is roughly 10,000 sq cm/sec in the upper troposphere, PH3 should be depleted there with a scale height of about 3.5 km. An upper limit of 100,000 sq cm/sec is estimated for K. If the gas phase concentration of P2H4 can be neglected, production of molecular phophorus is very unlikely unless the spin-forbidden recombination reaction PH+H2+M - PH3+M occurs with an exceptionally low rate. Coupling of PH3 and hydrocarbon photochemistries is very important. Possible observable amounts of the organophosphorus molecules CH3PH2 and HCP are tentatively predicted.

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