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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 7.

Energies of Saturn’s ℓ ∼ m f-modes as a function of the angular wavenumber ℓ. Black dots are observed modes from V. M. Afigbo et al. (2025). The curves show predicted energies for rotating and nonrotating convective excitation and the damping rates shown in Figure 3. Convective excitation cannot account for the observed mode energies.

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