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Figure 14 | Earth, Planets and Space

Figure 14

From: Idealized numerical experiments on microscale eddies in the Venusian cloud layer

Figure 14

Horizontal distributions (a,b; upper panels) and amplitudes of Fourier components (c,d; lower panels) of potential temperature. These are plots of eddy components of wind (m · s–1; arrows) and potential temperature (K; shaded) at 54 km under the condition U Z  = 0 m · s–1 · km–1 at (a) 40 min for case A10L and (b) 180 min for case B3L. Black and gray marks in (c,d) show amplitudes of potential temperatures in cases A10L and B3L and in cases A10 and B3, respectively.

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