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Twelve-Year Cycle in the Cloud Top Winds Derived from VMC/Venus Express and UVI/Akatsuki Imaging
DOI: 10.3390/atmos13122023 Bibcode: 2022Atmos..13.2023K

Titov, Dmitrij V.; Ignatiev, Nikolay I.; Khatuntsev, Igor V. +3 more

We present joint analysis of the UV (365 nm) images captured by the cameras on board ESA's Venus Express and JAXA's Akatsuki spacecraft. These observations enabled almost continuous characterization of the cloud top circulation over the longest period of time so far (2006-2021). More than 46,000 wind vectors were derived from tracking the UV cloud…

2022 Atmosphere
VenusExpress 5
Venus' Cloud-Tracked Winds Using Ground- and Space-Based Observations with TNG/NICS and VEx/VIRTIS
DOI: 10.3390/atmos13020337 Bibcode: 2022Atmos..13..337M

Machado, Pedro; Peralta, Javier; Silva, José E. +3 more

Characterizing the wind speeds of Venus and their variability at multiple vertical levels is essential for a better understanding of the atmospheric superrotation, constraining the role of large-scale planetary waves in the maintenance of this superrotation, and in studying how the wind field affects clouds' distribution. Here, we present cloud-tr…

2022 Atmosphere
VenusExpress 3
Venus Atmospheric Dynamics at Two Altitudes: Akatsuki and Venus Express Cloud Tracking, Ground-Based Doppler Observations and Comparison with Modelling
DOI: 10.3390/atmos12040506 Bibcode: 2021Atmos..12..506M

Widemann, Thomas; Machado, Pedro; Peralta, Javier +6 more

2021 Atmosphere
VenusExpress 13
Winds in the Lower Cloud Level on the Nightside of Venus from VIRTIS-M (Venus Express) 1.74 µm Images
DOI: 10.3390/atmos12020186 Bibcode: 2021Atmos..12..186G

Khatuntsev, Igor V.; Patsaeva, Marina V.; Zasova, Ludmila V. +2 more

2021 Atmosphere
VenusExpress 9
Validation of the IPSL Venus GCM Thermal Structure with Venus Express Data
DOI: 10.3390/atmos10100584 Bibcode: 2019Atmos..10..584S

Piccioni, Giuseppe; Tellmann, Silvia; Lebonnois, Sebastien +4 more

General circulation models (GCMs) are valuable instruments to understand the most peculiar features in the atmospheres of planets and the mechanisms behind their dynamics. Venus makes no exception and it has been extensively studied thanks to GCMs. Here we validate the current version of the Institut Pierre Simon Laplace (IPSL) Venus GCM, by means…

2019 Atmosphere
VenusExpress 11