Venus upper atmosphere revealed by a GCM: II. Model validation with temperature and density measurements

@inproceedings{Gilli2021VenusUA,
  title={Venus upper atmosphere revealed by a GCM: II. Model validation with temperature and density measurements},
  author={Gabriella Gilli and Thomas Navarro and S{\'e}bastien Lebonnois and Diogo Quirino and Vasco Gestosa da Silva and Aur{\'e}lien Stolzenbach and Franck Lef{\'e}vre and Gerald Schubert},
  year={2021}
}
Venus Atmospheric Dynamics at Two Altitudes: Akatsuki and Venus Express Cloud Tracking, Ground-Based Doppler Observations and Comparison with Modelling
We present new results of our studies of zonal and meridional winds in both hemispheres of Venus, using ground- and space-based coordinated observations. The results obtained from telescope
Venus’ Cloud-Tracked Winds Using Ground- and Space-Based Observations with TNG/NICS and VEx/VIRTIS
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
Local-time Dependence of Chemical Species in the Venusian Mesosphere
Observed chemical species in the Venusian mesosphere show local-time variabilities. SO2 at the cloud top exhibits two local maxima over local time, H2O at the cloud top is uniformly distributed, and

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