B. Marticorena et G. Bergametti, MODELING THE ATMOSPHERIC DUST CYCLE .1. DESIGN OF A SOIL-DERIVED DUSTEMISSION SCHEME, JOURNAL OF GEOPHYSICAL RESEARCH-ATMOSPHERES, 100(D8), 1995, pp. 16415-16430
A soil-derived dust emission scheme has been designed to provide an ex
plicit representation of the desert dust sources for the atmospheric t
ransport models dealing with the simulation of the desert dust cycle.
Two major factors characterizing the erodible surface are considered:
(1) the size distribution of the erodible loose particles of the soil
which controls the erosion threshold and the emission strength and (2)
the surface roughness which imposes the efficient wind friction veloc
ity acting on the erodible surface. These two parameters are included
in a formulation of the threshold wind friction velocity by adapting a
size-dependent parameterization proposed by Iversen and White (1982)
and by applying to the rough erodible surfaces a drag partition scheme
derived from Arya (1975). This parameterization of the threshold fric
tion velocity has been included in an horizontal flux equation propose
d by White (1979). This allows to attribute a specific production rate
to each soil size range for each type of surface. The dust flux F is
then considered as a fraction of the total horizontal flux G, the valu
e of the ratio F/G being imposed, at this time, by the soil clay conte
nt. In summary, the computed mass fluxes depend on the soil size distr
ibution, the roughness lengths, and the wind friction velocity. The di
fferent steps of this scheme have been independently validated by comp
arison with relevant experimental data. Globally, the agreement is sat
isfying, so that the dust fluxes could be retrieved with less uncertai
nties than those observed in previous simulations of the desert dust c
ycle.