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Fig. 2 | Earth, Planets and Space

Fig. 2

From: Super-rotation independent of horizontal diffusion reproduced in a Venus GCM

Fig. 2

Kinetic energy of horizontal wind per unit mass per unit wavenumber for T42L60 run. a Dependency on the damping time of horizontal diffusion at 70 km. b Dependency on the height for the case with 0.1 Earth days for the damping time of horizontal diffusion. Gradient of n−5/3 and n−3 are shown by solid lines. The analysed data is the final day of the numerical simulation

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