@comment{{This file has been generated by bib2bib 1.94}}
@comment{{Command line: /usr/bin/bib2bib --quiet -c 'not journal:"Discussions"' -c year=1997 -c $type="ARTICLE" -oc pub1997.txt -ob pub1997.bib}}
  author = {{Forget}, F. and {Pierrehumbert}, R.~T.},
  title = {{Warming Early Mars with Carbon Dioxide Clouds That Scatter Infrared Radiation}},
  journal = {Science},
  year = 1997,
  volume = 278,
  pages = {1273},
  doi = {10.1126/science.278.5341.1273},
  adsurl = {},
  adsnote = {Provided by the SAO/NASA Astrophysics Data System}
  author = {{Read}, P.~L. and {Collins}, M. and {Forget}, F. and {Fournier}, R. and 
	{Hourdin}, F. and {Lewis}, S.~R. and {Talagrand}, O. and {Taylor}, F.~W. and 
	{Thomas}, N.~P.~J.},
  title = {{A GCM climate database for mars: for mission planning and for scientific studies}},
  journal = {Advances in Space Research},
  year = 1997,
  volume = 19,
  pages = {1213-1222},
  abstract = {{The construction of a new database of statistics on the climate and
environment of the Martian atmosphere is currently under way, with the
support of the European Space Agency. The primary objectives of this
database are to provide information for mission design specialists on
the mean state and variability of the Martian environment in
unprecedented detail, through the execution of a set of carefully
validated simulations of the Martian atmospheric circulation using
comprehensive numerical general circulation models. The formulation of
the models used are outlined herein, noting especially new improvements
in various schemes to parametrize important physical processes, and the
scope of the database to be constructed is described. A novel approach
towards the representation of large-scale variability in the output of
the database using empirical eigenfunctions derived from statistical
analyses of the numerical simulations, is also discussed. It is hoped
that the resulting database will be of value for both scientific and
engineering studies of Mars' atmosphere and near-surface environment.
  doi = {10.1016/S0273-1177(97)00272-X},
  adsurl = {},
  adsnote = {Provided by the SAO/NASA Astrophysics Data System}
  author = {{Ockert-Bell}, M.~E. and {Bell}, J.~F. and {Pollack}, J.~B. and 
	{McKay}, C.~P. and {Forget}, F.},
  title = {{Absorption and scattering properties of the Martian dust in the solar wavelengths}},
  journal = {\jgr},
  keywords = {Planetology: Solar System Objects: Mars, Planetology: Solid Surface Planets: Rings and dust},
  year = 1997,
  volume = 102,
  pages = {9039-9050},
  abstract = {{A new wavelength-dependent model of the single-scattering properties of
the Martian dust is presented. The model encompasses the solar
wavelengths (0.3 to 4.3 {$\mu$}m at 0.02 {$\mu$}m resolution) and does not
assume a particular mineralogical composition of the particles. We use
the particle size distribution, shape, and single-scattering properties
at Viking Lander wavelengths presented by Pollack et al. [1995]. We
expand the wavelength range of the aerosol model by assuming that the
atmospheric dust complex index of refraction is the same as that of dust
particles in the bright surface geologic units. The new
wavelength-dependent model is compared to observations taken by the
Viking Orbiter Infrared Thermal Mapper solar channel instrument during
two dust storms. The model accurately matches afternoon observations and
some morning observations. Some of the early morning observations are
much brighter than the model results. The increased reflectance can be
ascribed to the formation of a water ice shell around the dust
particles, thus creating the water ice clouds which Colburn et al.
[1989], among others, have predicted.
  doi = {10.1029/96JE03991},
  adsurl = {},
  adsnote = {Provided by the SAO/NASA Astrophysics Data System}