Storms, Variability, and Multiple Equilibria on Hot Jupiters

Observations of hot-Jupiter atmospheres show large variations in the location of the hot spot and the amplitude of spectral features. Atmospheric flow simulations using the commonly employed forcing and initialization have generally produced a large, monolithic patch of nearly stationary hot area located eastward of the substellar point at high altitude. Here we perform high-resolution (T682) pseudospectral simulations that accurately capture small-scale eddies and waves inherent in hot-Jupiter atmospheres due to ageostrophy. The atmospheres contain a large number of intense storms over a wide range of scales, including the planetary scale. The latter sized storms dictate the large-scale spatial distribution and temporal variability of hot, as well as cold, regions over the planet. In addition, they exhibit quasi-periodic life cycles within multiple equilibrium states-all identifiable in the disk-integrated time series of the temperature flux.

Automated summary

Observations of hot-Jupiter atmospheres show significant variations in the hot spot location and spectral feature amplitude. High-resolution simulations reveal intense storms of various scales, influencing the spatial distribution and temporal variability of hot and cold regions over the planet. The quasi-periodic life cycles of storms in multiple equilibrium states are identifiable in the temperature flux time series.