The distribution of methylamine in the Jovian atmosphere | Zendy

Kuhn W. R. | Zendy; Atreya S. K. | Zendy; Chang S. | Zendy

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The distribution of methylamine in the Jovian atmosphere

Author(s) -

Kuhn W. R.,

Atreya S. K.,

Chang S.

Publication year - 1977

Publication title -

geophysical research letters

Language(s) - English

Resource type - Journals

SCImago Journal Rank - 2.007

H-Index - 273

eISSN - 1944-8007

pISSN - 0094-8276

DOI - 10.1029/gl004i005p00203

Subject(s) - jovian , methylamine , atmosphere of jupiter , mixing ratio , jupiter (rocket family) , atmosphere (unit) , production rate , ammonia , mixing (physics) , atmospheric sciences , physics , environmental science , astrobiology , astrophysics , astronomy , chemistry , meteorology , planet , industrial engineering , organic chemistry , space shuttle , quantum mechanics , saturn , engineering

An estimate of the methylamine concentration on Jupiter has been made. The maximum production rate of 6 × 10 4 cm −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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