Vertical Transport in the Jovian Upper Troposphere: Insights from Phosphine Submillimeter Observations

Astronomy and Astrophysics – Astronomy

Scientific paper

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Scientific paper

One-dimensional coupled photochemistry/transport model simulations of the phosphine profile in Jupiter's upper troposphere are compared with submillimeter observations. Adopting a stagnant atmosphere between 100 and approximately 400 mbar relative to the rate of mixing at higher pressures results in the best model simulations of the profiles derived from the observations.

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