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}
}
View PDF on arXiv
5 Citations
Background Citations
1
Methods Citations
1

5 Citations

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…
Venus mountain waves in the upper atmosphere simulated by a time-invariant linear full-wave spectral model
Venus’ upper atmosphere revealed by a GCM: I. Structure and variability of the circulation

References

SHOWING 1-10 OF 106 REFERENCES
The thermal structure of the Venus atmosphere: Intercomparison of Venus Express and ground based observations of vertical temperature and density profiles
Mesospheric vertical thermal structure and winds on Venus from HHSMT CO spectral-line observations
Upper atmosphere temperature structure at the Venusian terminators: A comparison of SOIR and VTGCM results
Models of Venus neutral upper atmosphere: Structure and composition
Wave analysis in the atmosphere of Venus below 100-km altitude, simulated by the LMD Venus GCM
Long term evolution of temperature in the venus upper atmosphere at the evening and morning terminators
Dayside thermal structure of Venus' upper atmosphere characterized by a global model
[1] Observations of Venus' dayside thermal structure are being conducted through ground based observatories. These temperature measurements, along with those from several instruments onboard the…
Update of the Venus density and temperature profiles at high altitude measured by SOIR on board Venus Express
Gravity waves in the upper atmosphere of Venus revealed by CO2 nonlocal thermodynamic equilibrium emissions
[1] The imaging capabilities of the Visible and Infrared Thermal Imaging Spectrometer-Mapper (VIRTIS-M) onboard Venus Express mission are used to analyze perturbations of CO2 nonlocal thermodynamic…
Venus upper atmosphere winds from ground-based heterodyne spectroscopy of CO2 at 10μm wavelength
...
...