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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 9.

Top: similar to Figure 8, but now showing the amplitude of each of Saturn’s ℓ ∼ m f-mode gravitational potential perturbations, δΦ/(GM/R), measured at the surface of Saturn. Bottom: the predicted gravitational perturbations of Saturn’s ℓ = 2 p-modes.

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