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}
}
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6 Citations
Background Citations
1
Methods Citations
1

6 Citations

Venus’ upper atmosphere revealed by a GCM: I. Structure and variability of the circulation

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…

Exploring the variability of the Venusian thermosphere with the IPSL Venus GCM

Venus mountain waves in the upper atmosphere simulated by a time-invariant linear full-wave spectral model

References

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Venus’ upper atmosphere revealed by a GCM: I. Structure and variability of the circulation

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