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• W1990147165 abstract "Possible interrelationships of different observations have been studied to clear up some obvious inconsistencies and develop a coherent picture of the kinematics of the Venus atmosphere. There is a wind shear in the vicinity of 60 km with vertical dimensions on the order of a scale height. The kinematical model has negligible surface winds, speeds increasing with altitude to approximately 45 km, a layer of high-speed retrograde zonal winds extending from approximately 45 to 60 km, a wind shear between 60 and 65 km, and slow atmospheric motions above this. Spacecraft data show that the region of high-speed winds is thicker on the day side of the planet than on the night side." @default.
• W1990147165 created "2016-06-24" @default.
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• W1990147165 date "1978-08-01" @default.
• W1990147165 modified "2023-10-05" @default.
• W1990147165 title "Vertical extent of zonal winds on Venus" @default.
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• W1990147165 doi "https://doi.org/10.1016/0019-1035(78)90003-9" @default.
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