A ground‐to‐exosphere Martian general circulation model: 1. Seasonal, diurnal, and solar cycle variation of thermospheric temperatures
By F. González-Galindo, Francois Forget, M. López‐Valverde, M. Coll, Ehouarn Millour. 2009
195 citations recorded by the source corpus.
Subfields: Astronomy and Astrophysics, Physiology
View Paper: https://www.semanticscholar.org/paper/389679a23bcbb750e39b730f0b9fa0af681f4912
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In Astronomy and Astrophysics
- Francois Forget
- Peter L Read
- J. Chaufray
- S. Lebonnois
- M. López‐Valverde
- F. González-Galindo
- G. Gilli
- François Leblanc
In Physiology
Citations in the corpus
- Three‐dimensional Martian ionosphere model: I. The photochemical ionosphere below 180 km (2013, methodology): “The temperature is higher in the evening terminator than in the morning terminator [see González-Galindo et al., 2009, Figure 3], inducing differences in the scale height and in the vertical distribution of the different species.”
- The Atmospheric Dynamics of Venus (2017, background): “…(TGCM, e.g. Bougher and Dickinson 1988; Bougher et al. 1990) modeling the atmospheric circulation above a given altitude level, or vertically extended GCMs that include these additional parameterizations, such as the LMD Mars GCM (e.g. Angelatsi-Coll et al. 2005; Gonzalez-Galindo et al. 2009).”