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The Atmospheric Dynamics of Venus
Sánchez-Lavega, Agustín; Imamura, Takeshi; Lebonnois, Sebastien +2 more
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 …
Solar Wind Interaction and Impact on the Venus Atmosphere
Barabash, Stas; Stenberg Wieser, Gabriella; Futaana, Yoshifumi +1 more
Venus has intrigued planetary scientists for decades because of its huge contrasts to Earth, in spite of its nickname of "Earth's Twin". Its invisible upper atmosphere and space environment are also part of the larger story of Venus and its evolution. In 60s to 70s, several missions (Venera and Mariner series) explored Venus-solar wind interaction…
Venus Surface Composition Constrained by Observation and Experiment
Helbert, Jörn; Gilmore, Martha; Treiman, Allan +1 more
New observations from the Venus Express spacecraft as well as theoretical and experimental investigation of Venus analogue materials have advanced our understanding of the petrology of Venus melts and the mineralogy of rocks on the surface. The VIRTIS instrument aboard Venus Express provided a map of the southern hemisphere of Venus at ∼1 µm…
Heliosheath Processes and the Structure of the Heliopause: Modeling Energetic Particles, Cosmic Rays, and Magnetic Fields
Wurz, P.; Fichtner, H.; Scherer, K. +11 more
This paper summarizes the results obtained by the team "Heliosheath Processes and the Structure of the Heliopause: Modeling Energetic Particles, Cosmic Rays, and Magnetic Fields" supported by the International Space Science Institute (ISSI) in Bern, Switzerland. We focus on the physical processes occurring in the outer heliosphere, especially at i…
Aeronomy of the Venus Upper Atmosphere
Pätzold, M.; López-Valverde, M. A.; Drossart, P. +3 more
We present aeronomical observations collected using remote sensing instruments on board Venus Express, complemented with ground-based observations and numerical modeling. They are mostly based on VIRTIS and SPICAV measurements of airglow obtained in the nadir mode and at the limb above 90 km. They complement our understanding of the behavior of Ve…