Kelvin waves over a differentially rotating spherical shell

Open Access

Fig. 5.

Frequency difference Δω = ω_m + 1 − ω_m between two consecutive Kelvin modes as a function of core radius. Red dots show the values for the full sphere case as derived from (C.10), while the dashed black line shows the asymptotic shallow-water case. Parameters are γ = 1, E = 10⁻³ with N_r = L_max = 20.

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