Physics
Scientific paper
Feb 1993
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993jgr....98.3197m&link_type=abstract
Journal of Geophysical Research (ISSN 0148-0227), vol. 98, no. E2, p. 3197-3220.
Physics
41
Atmospheric Models, Dust Storms, Mars Atmosphere, Planetary Meteorology, Opacity, Particle Size Distribution, Mars, Storms, Dust, Simulations, Zones, Numerical Methods, Transport, Size, Particles, Atmosphere, Model, Aerosols, Surface, Latitude, Dynamics, Opacity, Spacecraft Observations, Mariner 9 Mission, Shape, Iris Instrument, Distribution, Radiative Effects, Physical Properties, Mixing, Landing Sites, Origin, Source
Scientific paper
A zonally symmetric primitive-equation grid-point model of the Martian atmosphere is coupled with an aerosol transport/microphysical model in order to numerically investigate the size-dependent transport of dust particles in the Martian atmosphere. The coupled model accounts for diabatic heating due to a radiatively active evolving dust field, but neglects feedbacks between atmosphere-surface interactions and surface dust lifting. The differing suspension lifetimes of dust particles of various sizes (radius = 1-80 microns), in conjunction with spatially varying atmospheric dynamics, result in latitudinal differences in several measurements of the column integrated particle concentration. This work indicates the importance of considering the full range of particle sizes (and shapes) of the suspended dust during Martian global dust storms and their impact upon the spatial extent and wavelength-dependent radiative influence of such storms.
Haberle Robert M.
Murphy Ronald J.
Pollack James B.
Toon Brian O.
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