Differential rotation may greatly enhance convective viscosity in giant planets, making f-mode and p-mode damping times long enough that storms and impacts can excite detectable oscillation amplitudes.
R., Barik, A., & Fuller, J
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Excitation and Damping of Oscillation Modes in Gaseous Planets
Differential rotation may greatly enhance convective viscosity in giant planets, making f-mode and p-mode damping times long enough that storms and impacts can excite detectable oscillation amplitudes.