Results 1 to 10 of about 4,918 (242)

Sulfur monoxide dimer chemistry as a possible source of polysulfur in the upper atmosphere of Venus. [PDF]

Nat Commun, 2021
Pinto JP, Li J, Mills FP, Marcq E, Evdokimova D, Belyaev D, Yung YL.   +6 more
europepmc   +3 more sources

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, Sebastien Lebonnois, Takeshi Imamura   +2 more
exaly   +3 more sources

The Effect of Recent Venus Transit on Earth’s Atmosphere

Annals of Geophysics, 2006
Some experiments on June 8, 2004, the day of transit of Venus across the Sun, were undertaken at Kolkata (latitude: 23034? N) to observe effect, if any, of transit of Venus on FWF, ELF and VLF amplitudes.
H. P. Sardar, S. K. Mandal, P. K. Mandal, A. Guha, S. K. Sarkar, B. K. Sarkar, S. K. Adhikari, B. K. De, S. S. De, M. Ray   +9 more
doaj   +5 more sources

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, Rainer Haus, Gabriele Arnold, Mario D’Amore, Alessandro Maturilli, Thomas Säuberlich, Harald Hiesinger   +6 more
doaj   +2 more sources

Life on Venus? [PDF]

Life
Venus 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
doaj   +2 more sources

Redox state of Earth’s magma ocean and its Venus-like early atmosphere [PDF]

Science Advances, 2020
Paolo A Sossi, Antony Burnham, James Badro   +2 more
exaly   +2 more sources

Mountain Waves in the Upper Atmosphere of Venus

Geophysical Research Letters
Planetary‐scale mountain waves have been observed at the cloud top of Venus and throughout the cloud deck. As they propagate from the surface to the cloud layers, multiple observations and numerical simulations have shown that they grow in size and do ...
T. Navarro, G. Schubert
doaj   +2 more sources

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
doaj   +1 more source

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
doaj   +1 more source

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, C. Osácar, A. Fernández-Pacheco   +2 more
doaj   +1 more source