The distribution of methylamine in the Jovian atmosphere

Physics

Scientific paper

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Amines, Atmospheric Chemistry, Atmospheric Composition, Jupiter Atmosphere, Methyl Compounds, Ammonia, Hydrocarbons, Photochemical Reactions, Photodissociation

Scientific paper

An estimate has been made of the methylamine concentration in the Jupiter atmosphere on the basis of the possible overlap between the regions of hydrocarbon and ammonia photochemistry. It was found that the maximum production rate of 6 x 10 to the 4th/cu cm/Jovian day occurs in the vicinity of 60 km above the ammonia cloud layer. The volumetric mixing ratio is 3 x 10 to the -11th, if the downward transport of methylamine equals the production rate.

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