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Temperature, cloud structure, and dynamics of venus middle atmosphere by infrared remote sensing from pioneer orbiter
Authors:Taylor F W  Diner D J  Elson L S  McCleese D J  Martonchik J V  Delderfield J  Bradley S P  Schofield J T  Gille J C  Coffey M T
Abstract:Further results from the Venus orbiter radiometric temperature experiment (VORTEX) on the Pioneer orbiter are presented. These are used to characterize the three-dimensional temperature field, the cloud structure, and the dynamics of the 60-to 130-kilometer altitude region of the Venus atmosphere. One of the new discoveries is a "dipole" structure at high latitudes, with two hot spots rotating around the pole, surrounded by banks of cold cloud.
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