Variable winds on Venus mapped in three dimensions

By A. Sánchez‐Lavega, Ricardo Hueso, G. Piccioni, P. Drossart, J. Peralta, S. Pérez-Hoyos, C. Wilson, Frank Taylor, K. Baines, D. Luz and 2 more. 2008

156 citations recorded by the source corpus.

Subfields: Astronomy and Astrophysics, Physiology

View Paper: https://www.semanticscholar.org/paper/eef6a76681df577740a1ff3f17c13846deec9736

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In Astronomy and Astrophysics

1. S. Lebonnois
2. N. Ignatiev
3. V. Wilquet
4. Peter L Read
5. K. McGouldrick
6. D. Titov

Citations in the corpus

• Clouds and Hazes of Venus (2018, background): “The middle and high latitudes are also characterized by vanishing vertical wind shear within the clouds (Sánchez-Lavega et al. 2008) that suppresses wind shear instabilities.”
• The Atmospheric Dynamics of Venus (2017, methodology): “Even allowing for the variability represented in the ensemble of measurements, ranging from Mariner 10 to Venus Express VIRTIS and VMC, the low latitude peak in m is quite broad and flat with relatively steep latitudinal gradients poleward of 40◦–50◦ in each hemisphere, especially at the top of the ”