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Excitation and Damping of Oscillation Modes in Gaseous Planets

  • Authors: Jim Fuller, Marzia Parisi, Steve Markham, A. James Friedson, J. R. Fuentes

Jim Fuller et al 2026 The Planetary Science Journal 7 .

  • Provider: AAS Journals

Caption: Figure 2.

The damping time of ℓ = m f-modes in Saturn, as a function of the angular number ℓ, due to different models of convective viscosity. The blue line shows the simple estimate of Equation (4), while the green line accounts for enhancement due to zonal winds (Equation (12)).

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