Results 101 to 110 of about 4,918 (242)

The upper atmosphere of Venus: Model predictions for mass spectrometry measurements

, 2019
Salome Gruchola, André Galli, Audrey Vorburger, P. Wurz   +3 more
openalex   +2 more sources

Evidence for carbonyl sulfide (OCS) conversion to CO in the lower atmosphere of Venus [PDF]

, 2009
Yuk L. Yung, Mao‐Chang Liang, Xun Jiang, Run‐Lie Shia, C. Lee, Bruno Bézard, Emmanuel Marcq   +6 more
openalex   +1 more source

TRAPPIST-1 d: Exo-Venus, Exo-Earth, or Exo-Dead?

The Astrophysical Journal Letters
TRAPPIST-1 d is generally assumed to be at the boundary between a Venus-like world and an Earth-like world, although recently published works on TRAPPIST-1 b and c raise concerns that TRAPPIST-1 d may be similarly devoid of a substantial atmosphere ...
M. J. Way
doaj   +1 more source

Prediction of Sulfate Hazes in the Lower Venus Atmosphere

The Planetary Science Journal
We study the amount, size distribution, and material composition of submicron aerosol particles in the lower Venus atmosphere
Peter Woitke, Manuel Scherf, Christiane Helling, Paul Rimmer, Martin Ferus, Helmut Lammer, Fabian Weichbold, Kateřina Němečková, Petr Eminger, Jaroslav Kačina, Tereza Constantinou   +10 more
doaj   +1 more source

Is OSSO a Significant Contributor to the Unknown UV Absorber in Venus' Atmosphere?

Geophysical Research Letters
It has been proposed that two isomers of the SO dimer (cis‐ and trans‐OSSO) are candidates for the unknown UV absorber in Venus' atmosphere because they have a good spectral match with the absorber, despite the low concentrations predicted by 1D ...
Joanna V. Egan, Wuhu Feng, Alexander D. James, James Manners, Daniel R. Marsh, Sébastien Lebonnois, Franck Lefèvre, Aurélien Stolzenbach, John M. C. Plane   +8 more
doaj   +1 more source

New Analysis Provides a Fresh View of the Atmosphere on Venus

, 2019
Aaron Sidder
openalex   +1 more source

Planetary Waves Drive Horizontal Variations in Trace Species in the Venus Deep Atmosphere

The Planetary Science Journal
The deep atmosphere of Venus remains mysterious because of the planet’s high, optically thick cloud decks. While phenomena such as the observed decadal fluctuations in sulfur dioxide abundance above the clouds could shed light on conditions below, poor ...
Maureen Cohen, James Holmes, Stephen Lewis, Manish Patel   +3 more
doaj   +1 more source

Further Studies of the Circulation of the Venus Atmosphere [PDF]

, 1989
Arthur Y. Hou, R. M. Goody
openalex   +1 more source

Dynamics of the Four-Day Circulation in the Venus Atmosphere

, 1980
Yuichi Matsuda
openalex   +2 more sources

Two-dimensional time-dependent model of the transport of minor species in the Venus night side upper atmosphere

, 2010
Arnaud Collet, Cédric Cox, Jean‐Claude Gérard   +2 more
openalex   +2 more sources