Atmospheric Circulation of Close-in Extrasolar Giant Planets: The Diabatic Equivalent-barotropic Model
We extend the description of equivalent-barotropic equations for exoplanets to the diabatic case—that is, with explicit heating and/or cooling representation, rather than with a stationary deflection of the bottom bounding surface. In the diabatic case, the equation for potential temperature (or ent...
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| Main Authors: | , , |
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| Format: | Article |
| Language: | English |
| Published: |
IOP Publishing
2025-01-01
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| Series: | The Astrophysical Journal |
| Subjects: | |
| Online Access: | https://doi.org/10.3847/1538-4357/ade9b9 |
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