Abstract
The deep atmosphere of Venus ( ∼ 180 km including the thermosphere) presents both observational and modeling challenges. Its thick, nearly uniform global cloud cover makes it difficult to fathom the vertical structure of the global circulation through available techniques that are applied to Earth’s atmosphere. Further, the slow rotation of the planet and the consequential prevailing cyclostrophic balance restricts easy inferences about the meridional flow and circulation (Gierasch et al. 1997, Read 1986, Schubert et al. 2007).
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Limaye, S.S., Rengel, M. (2013). Atmospheric Circulation and Dynamics. In: Bengtsson, L., Bonnet, RM., Grinspoon, D., Koumoutsaris, S., Lebonnois, S., Titov, D. (eds) Towards Understanding the Climate of Venus. ISSI Scientific Report Series, vol 11. Springer, New York, NY. https://doi.org/10.1007/978-1-4614-5064-1_5
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