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The Atmospheric Dynamics of Venus [PDF]
Space Science Reviews, 2017 We review our current knowledge of the atmospheric dynamics of Venus prior to the Akatsuki mission, in the altitude range from the surface to approximately the cloud tops located at about 100 km altitude. The three-dimensional structure of the wind field in this region has been determined with a variety of techniques over a broad range of spatial and ...
Agustín Sánchez-Lavega +2 more
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The second Venus flyby of BepiColombo mission reveals stable atmosphere over decades [PDF]
Nature Communications, 2023 Studies of the Venusian mesosphere provide important information about the current state of the entire Venusian atmosphere. This includes information about the dense cloud structure, its vertical thermal profile, temperature fields, and the resulting ...
Jörn Helbert +6 more
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LifeVenus is not generally at the forefront when considering extraterrestrial life. Yet, based on the physical similarities and proximity to Earth and with the little knowledge of its evolutionary history, there is a possibility that Venus may have hosted ...
Sanjay S. Limaye
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Comparison of the greenhouse effect between Earth and Venus using multiple atmospheric layer models [PDF]
E3S Web of Conferences, 2020 To better understand the mechanisms of global warming, we developed a one atmospheric layer model for Earth and a multiple atmospheric layer model (N = 111) for Venus.
Liu William Song
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Ammonia and Phosphine in the Clouds of Venus as Potentially Biological Anomalies
Aerospace, 2022 We are of the opinion that several anomalies in the atmosphere of Venus provide evidence of yet-unknown processes and systems that are out of equilibrium.
Carol E. Cleland, Paul B. Rimmer
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Brief communication: Lower-bound estimates for residence time of energy in the atmospheres of Venus, Mars and Titan [PDF]
Nonlinear Processes in Geophysics, 2021 The residence time of energy in a planetary atmosphere, τ, which was recently introduced and computed for the Earth's atmosphere (Osácar et al., 2020), is here extended to the atmospheres of Venus, Mars and Titan.
J. Pelegrina +2 more
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Generation of gravity waves from thermal tides in the Venus atmosphere
Nature Communications, 2021 Gravity waves are observed in Venus atmosphere, but their characteristics are not well-known. Here, the authors show spontaneous generation of gravity waves from the thermal tides in the Venus atmosphere as small-scale gravity waves are resolved in high ...
Norihiko Sugimoto +6 more
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Venus: A planetary window into early Earth
地球与行星物理论评, 2022 Venus is the most similar planet to the Earth in the solar system in terms of planet size, mass and orbital velocity. Since the early 1960s, Venus has been an important target for human deep space exploration.
Le Chen, Shao-Bing Zhang, Jin-Fei Yu
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Remote Sensing, 2023 Understanding crust–atmosphere interactions on Venus is fundamentally important to interpretations of Venus’ surface spectroscopic data. Olivine, in basaltic crust, is oxidized under a heated CO2 atmosphere.
Shan-Shan Zhong +12 more
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Aerospace, 2022 Recent and past observations of chemical and physical peculiarities in the atmosphere of Venus have renewed speculations about the existence of life in its clouds.
Niels F. W. Ligterink +8 more
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