Astronomy and Astrophysics – Astronomy
Scientific paper
Jul 1997
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1997dps....29.2405a&link_type=abstract
American Astronomical Society, DPS meeting #29, #24.05; Bulletin of the American Astronomical Society, Vol. 29, p.1017
Astronomy and Astrophysics
Astronomy
Scientific paper
There is no known chemical source of phosphine in the Jovian upper troposphere. Its presence in the upper atmosphere therefore is the result of upward transport from the interior. The retrieval of the vertical profile of phosphine in the upper troposphere from ground-based submillimeter observations provides then an opportunity to derive the magnitude of dynamical mixing in this altitude range. Using the Caltech/JPL Jovian 1-D coupled chemistry/transport model, we find that the phosphine measurements provide evidence for rapid mixing at pressures greater than 330 mbar and a stagnant layer above. As the measurements are globally-averaged, the model simulation also is for the mean global atmosphere.
Allen Marsha M.
Lee Yin-Tat
Serabyn Eugen
Weisstein Eric Wolfgang
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