Fig. 13.

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Equatorial power spectrum of latitudinal velocity vθ near the surface r = 0.95 R⊙. The spectra are computed in a frame rotating at Ω0/2π = 431.3 nHz. The blue solid line represents the differential rotation rate at the surface ω = m(Ωsf − Ω0) where Ωsf = ⟨Ω(0.95 R⊙, π/2)⟩. The red points denote the theoretical dispersion relation of the sectoral Rossby modes, ω = −2Ωsf/(m + 1)+m(Ωsf − Ω0).
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