Weak Jets and Strong Cyclones: Shallow-Water Modeling of Giant Planet Polar Caps

Giant planet tropospheres lack a solid, frictional bottom boundary. The troposphere instead smoothly transitions to a denser fluid interior below. However, Saturn exhibits a hot, symmetric cyclone centered directly on each pole, bearing many similarities to terrestrial hurricanes. Transient cyclonic...

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Bibliographic Details
Main Authors: O'Neill, Morgan E (Contributor), Emanuel, Kerry Andrew (Contributor), Flierl, Glenn Richard (Contributor)
Other Authors: Massachusetts Institute of Technology. Department of Earth, Atmospheric, and Planetary Sciences (Contributor)
Format: Article
Language:English
Published: American Meteorological Society, 2018-04-05T15:46:22Z.
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