Digital Database of Modern Evaporites and their Predicted Distribution Based on Results...
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Fig.6 The distribution of two subsets of the Cogley (1991) GGHYDRO database. Cogley's
(1991) SFLT (salt flats) and SLTW (salt water) filtered to remove oceans and inland seas
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Conclusions
The new database of modern evaporites consists of digitized polygons, points, and
fractional coverage data representing both naturally occurring and man-made
(solar salt operations) evaporites. The new database is a significant improvement
over the previous evaporite database (Cogley 1991) because it more accurately
represents the actual distribution of evaporites, and subdivides them into: (1)
non-marine saline pans and saline mudflats; (2) non-marine saline lakes; and (3)
marginal marine sabkhas and salinas. The mean latitude of evaporites in the
Northern Hemisphere is 33SN with a standard deviation of 11.3°. The mean latitude of evaporites in the Southern Hemisphere is 27.6°S with a standard deviation
of 7.0°. This represents a shift of the mean latitude of evaporites by approximately
3° north of 30° latitude in both hemispheres. This is most likely due to a meteorological thermal equator that lies a few degrees north of the geographic equator.
The majority of large, Phanerozoic evaporite deposits were formed in basins
along continental margins with restricted marine connections. The present-day
evaporites most likely to be preserved in the geologic record are the marginal marine evaporites centered near 30 0 N and 30 0 S latitude. Although the marginal marine
evaporites represent a very small portion of the total present-day evaporites, their
distribution closely approximates the mean latitudes of all modern evaporites.
Most of the observed evaporites between 30 0 N and 30 0 S latitude were predicted by the proxy formation model using 12-month (mean annual) forcing from
the GENESIS (2.0) simulation of present-day climate.
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