Some fundamental questions concerning the circulation of the atmosphere of Venus
References (3)
There are more references available in the full text version of this article.
Cited by (5)
Radio science investigations by VeRa onboard the Venus Express spacecraft
2006, Planetary and Space ScienceVenus microsat explorer programme, an ESA technology reference study
2006, Acta AstronauticaVenus Entry Probe Technology Reference Study
2006, Advances in Space ResearchCitation Excerpt :Venus has a very complicated atmospheric dynamical system. The driving force behind the zonal super rotation, the dynamics of the polar vortices, and the meridional circulation as well as the cause of temporal and spatial variations of the cloud layer opacity are all rather poorly understood (Moroz, 2002; Taylor, 2002; Titov et al., 2002). [MO4] Aerosols in the cloud layers
The energy cascade in a strongly stratified fluid
2006, Journal of Fluid MechanicsStructure of the Venus neutral atmosphere as observed by the Radio Science experiment VeRa on Venus Express
2009, Journal of Geophysical Research: Planets
Copyright © 2002 Published by Elsevier Ltd.