Figure 2From: Idealized numerical experiments on microscale eddies in the Venusian cloud layerInitial vertical profiles of (a) potential temperature (K) and (b) passive tracer (kg · kg–1). The potential temperature difference from 350 K at 51 km is 0 K for cases B1 to B5, 0.8 K for case A02, 2 K for case A05, 4 K for case A10, 8 K for case A20, and 12 K for case A30.Back to article page