A database of statistics which describe the climate and surface environment
of Mars has been constructed directly on the basis of output from multiann
ual integrations of two general circulation models developed jointly at Lab
oratoire de Meteorologie Dynamique du Centre National de la Recherche Scien
tifique, France, and the University of Oxford, United Kingdom, with support
from the European Space Agency. The models have been developed and validat
ed to reproduce the main features of the meteorology of Mars, as observed b
y past spacecraft missions. As well as the more standard statistical measur
es for mission design studies, the Mars Climate Database includes a novel r
epresentation of large-scale variability, using empirical eigenfunctions de
rived from an analysis of the full simulations, and small-scale variability
using parameterizations of processes such as gravity wave propagation. The
database may be used as a tool for mission planning and also provides a va
luable resource for scientific studies of the Martian atmosphere. The datab
ase is described and critically compared with a representative range of cur
rently available observations.