Acceleration of superrotation in simulated hot Jupiter atmospheres

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Fig. C.2

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Temperature (colors) and winds (arrows), both in arbitrary unit, as a function of longitude and latitude for the shallow water solutions of Eqs. (40) and (A.7) considering τ_rad = 2.8 and τ_drag = 28. Presenting (a) westward propagating gravity wave; (b) Rossby wave; and (c) Kelvin wave.

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