Atmospheres of Hot Rocky Planets with Ultra-Short Orbital Period
Investigating atmospheric circulation of hot rocky exoplanets using non-grey GCM simulations with custom correlated-k coefficients.
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Investigating atmospheric circulation of hot rocky exoplanets using non-grey GCM simulations with custom correlated-k coefficients.
We use the ExoCAM GCM to investigate the inner edge of the habitable zone around white dwarfs, finding a novel "bat rotation" regime.