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Slantwise convection on fluid planets

GEOPHYSICAL RESEARCH LETTERS, no. 20 (2016): 10611-10620

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Abstract

Slantwise convection should be ubiquitous in the atmospheres of rapidly rotating fluid planets. We argue that convectively adjusted lapse rates should be interpreted along constant angular momentum surfaces instead of lines parallel to the local gravity vector. Using Cassini wind observations of Jupiter and different lapse rates to constr...More

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