Mars experiment
Model
Model description
- Primitive equation system
- Mars atmosphere radiation model
- Turbulent mixing (Mellor and Yamada (1982) level 2.5)
- Surface flux (Beljaars and Holtslag, 1991)
- Simple land model (bucket model, soil heat diffusion)
- Convective adjustment (e.g., Manabe et al., 1965)
Setting and result
MGS scenario, T21L36
- Dust distribution: MGS scenario (Forget et al., 2001)
- Used data
- Resolution: T21L36
- Integration time: 5 Mars years
- namelist file
- Result
Visualization program & scripts
- Programs & scripts (Japanese only)
References
- Forget, F., Y. Wanherdrick, and S. R. Lewis (2001), Validation of the Mars General Circulation Model and Climate Database with new spacecraft observations, in Work Package 7, Tech. Note 11369/95/NL/JG, Eur. Space Agency, Paris. (Available at <URL:http://www-mars.lmd.jussieu.fr/mars/esadoc/lmd/esadoc.html>.)
- Forget, F., F. Hourdin, R. Fournier, C. Hourdin, and O. Talagrand (1999), Improved general circulation models of the Martian atmosphere from the surface to above 80 km, J. Geophys. Res., 104, 24155.