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Figure 4 | Earth, Planets and Space

Figure 4

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

Figure 4

Time-height cross sections of area-mean θ w ¯ (upper panels) and q w ¯ (lower panels). These fluxes normalized by maximum flux magnitudes in Figure 3 are calculated from the experiments under the condition U Z  = 0 m · s–1 · km–1 for (a) case A02, (b) case A10, and (c) case A20. Thick contours in upper and lower panels show area-mean potential temperature (K) and mixing ratio (q × 106; kg · kg–1), respectively. Thin-dashed contours indicate negative values of normalized θ w ¯ .

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