1977•Geophysical Research LettersRequires access

The distribution of methylamine in the Jovian atmosphere

William R. Kuhn, S. K. Atreya, S. Chang

Open publisher page 25 citations

Abstract

An estimate of the methylamine concentration on Jupiter has been made. The maximum production rate of 6 × 104cm−3 (Jovian day)−1 occurs in the vicinity of 60 km above the ammonia cloud layer. If the downward transport of methylamine equals the production rate, then the volumetric mixing ratio is 3 × 10−11.

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An estimate of the methylamine concentration on Jupiter has been made. The maximum production rate of 6 × 104cm−3 (Jovian day)−1 occurs in the vicinity of 60 km above the ammonia cloud layer. If the downward transport of methylamine equals the production rate, then the volumetric mixing ratio is 3 × 10−11.

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Available abstract

An estimate of the methylamine concentration on Jupiter has been made. The maximum production rate of 6 × 104cm−3 (Jovian day)−1 occurs in the vicinity of 60 km above the ammonia cloud layer. If the downward transport of methylamine equals the production rate, then the volumetric mixing ratio is 3 × 10−11.

Key concepts: Jovian, Methylamine, Atmosphere of Jupiter, Mixing ratio, Jupiter (rocket family), Atmosphere (unit), Production rate, Ammonia

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