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

  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},

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



Upper atmosphere temperature structure at the Venusian terminators: A comparison of SOIR and VTGCM results

Thermal structure of the upper atmosphere of Venus simulated by a ground-to-thermosphere GCM

Models of Venus neutral upper atmosphere: Structure and composition

Thermal structure of Venusian nighttime mesosphere as observed by VIRTIS‐Venus Express

[1] The mapping IR channel of the Visual and Infrared Thermal Imaging Spectrometer (VIRTIS-M) on board the Venus Express spacecraft observes the CO2 band at 4.3 μm at a spectral resolution adequate

A photochemical model for the Venus atmosphere at 47–112 km

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