A popular technique in paleoclimatology is the definition of occurrences of
climate-sensitive lithofacies, such as evaporite deposits, using a global
grid system. The simplest and most widely used grid systems in paleoclimato
logy are orthogonal grids that use lines of latitude and longitude as grid-
cell boundaries. Occurrences defined using orthogonal grids, however, can d
iffer greatly in size and shape because lines of longitude converge at the
poles, distorting the shape of the grid system. As a result of this distort
ion, the latitude at which the occurrences were defined can affect the numb
er and distribution of occurrences. As an alternative, spherical geodesic s
ystems can be used. Spherical geode sic systems have near-equal area and ne
ar-equal shape grid-cells for the entire sphere, which significantly reduce
biases introduced by the grid system. Spherical geodesic systems can make
paleoclimatic studies using occurrences of climate-sensitive lithofacies mo
re reliable. To make spherical geodesic systems practical for paleoclimate
applications, a "tool kit" of programs written in C has been assembled. Fou
r programs are included in the tool kit: DESIGNER, which designs spherical
geodesic grids, PLOTTER, which generates import files for Terra Mobilis(TM)
and PGIS/Mac(TM) to display the grids, MAPPER, which defines occurrences u
sing the grids, and ROTATOR, which rotates data about Euler poles. Middle D
evonian evaporite data for North America were compiled to demonstrate each
of the functions. (C) 1998 Elsevier Science Ltd. All rights reserved.