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Fig. 4.

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Comparison of two gravito-inertial modes along ϕ = 0 for the different formulations. The first mode, with ω ̂ = 0.421 N $ \hat{\omega}=0.421 N $, corresponds to the 1g22 mode impacted by the rotation, while the second one is closer to an inertial or gravito-inertial mode, ω ̂ = 0.777 N $ \hat{\omega}=0.777 N $. Velocities are given in units such that Roωd = 1.56 × 1010 cm s−1. Left: Toroidal velocity uϕ at ϕ = 0 for ω ̂ = 0.421 N $ \hat{\omega}=0.421 N $ in the full formulation (Panel a), split formulation (Panel b) and with only effective Coriolis forcing (Panel c). Right: Toroidal velocity uϕ at ϕ = 0 for ω ̂ = 0.777 N $ \hat{\omega}=0.777 N $ in the full formulation (Panel a), split formulation (Panel b) and with only effective Coriolis forcing (Panel c).

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