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R. John Wilson


Middle Atmosphere Dynamics and Chemistry; Planetary Atmosphere Dynamics
Geophysical Fluid Dynamics Laboratory
National Oceanic and Atmospheric Administration
P. O. Box 308, Princeton, NJ 08542 USA


Program in Atmospheric and Oceanic Sciences
Princeton University

email: John.Wilson@noaa.gov
phone: 609-452-6592
FAX: 609-987-5063


Research Interests


Mars Atmosphere Modeling and Observation Workshop: Granada, Spain, 2006


Mars Atmosphere Modeling and Observation Workshop: Granada, Spain, 2003


Manuscripts in preparation or submitted for publication

Publications

Journals, Preprint servers, meetings etc

Other home pages





A GCM simulation of the early stage of a Martian great dust storm. The data is displayed in a latitude-longitude projection with the northernmost latitude running along the front edge of the picture. The general upslope of topography from the Northern Hemisphere to the Southern Hemisphere is evident along the left edge of the picture. The smaller of the two dust plumes is rising up from the western slope of the Hellas basin and continues into the eastern hemisphere as a distinct entity from the plume rising from the southern portion of the Tharsis plateau.
(from Wilson and Hamilton, 1996) (PDF)

Other figures:


A GCM simulation of the dispersion of particles initially confined within the vicinity of the summer hemisphere polar cap. The simulation tracks 25000 particles that are color-coded by their initial latitude.
R.J. Wilson, M.I. Richardson, R.T. Clancy and A.V. Rodin 1997: Simulation of Aerosol and Water Vapor Transport with the GFDL Mars General Circulation Model. Bull. Amer. Astron. Society )


Misc






R. John Wilson(John.Wilson@noaa.gov)
last modified:May 15 2008.