Incorporation of a gravity wave momentum deposition parameterization into the Venus Thermosphere General Circulation Model (VTGCM)

Author:

Zalucha A. M.1,Brecht A. S.2,Rafkin S.3,Bougher S. W.4,Alexander M. J.5

Affiliation:

1. SETI Institute; Mountain View California USA

2. NASA Ames Research Center; Moffett Field California 94035 USA

3. Department of Space Studies; Southwest Research Institute; Boulder Colorado USA

4. Department of Atmospheric, Oceanic, and Space Sciences; University of Michigan; Ann Arbor Michigan USA

5. NorthWest Research Associates - CoRA; 3380 Mitchell Lane Boulder Colorado USA

Funder

NASA Venus Express Participating Scientist Program

Publisher

American Geophysical Union (AGU)

Subject

Space and Planetary Science,Earth and Planetary Sciences (miscellaneous),Geochemistry and Petrology,Geophysics

Reference64 articles.

1. A mechanism for the Venus thermospheric superrotation;Alexander;Geophys. Res. Lett.,1992

2. A spectral parameterization of mean-flow forcing due to breaking gravity waves;Alexander;J. Atmos. Sci.,1999

3. Near infrared imaging spectroscopy of Venus with the Anglo-Australian Telescope;Bailey;Planet. Space Sci.,2008

4. Space-time relationships in the UV markings on Venus;Belton;J. Atmos. Sci.,1976a

5. Cloud patterns, waves, and convection in the Venus atmosphere;Belton;Bulletin of the American Astronomical Society, Bulletin of the American Astronomical Society,1976b

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