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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 3.

The damping time of ℓ = m f-modes of Saturn as a function of ℓ. The green line is damping due to convective viscosity (Equation (14)), the maroon line accounts for damping via interaction with the rings (Equation (15)), and the black line is the combined effect of both.

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