lmd_Li1993.bib
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@article{1993Sci...262.1252C,
author = {{Cess}, R.~D. and {Zhang}, M.-H. and {Potter}, G.~L. and {Barker}, H.~W. and
{Colman}, R.~A. and {Dazlich}, D.~A. and {del Genio}, A.~D. and
{Esch}, M. and {Fraser}, J.~R. and {Galin}, V. and {Gates}, W.~L. and
{Hack}, J.~J. and {Ingram}, W.~J. and {Kiehl}, J.~T. and {Lacis}, A.~A. and
{Le Treut}, H. and {Li}, Z.-X. and {Liang}, X.-Z. and {Mahfouf}, J.-F. and
{McAvaney}, B.~J. and {Meleshko}, V.~P. and {Morcrette}, J.-J. and
{Randall}, D.~A. and {Roeckner}, E. and {Royer}, J.-F. and {Sokolov}, A.~P. and
{Sporyshev}, P.~V. and {Taylor}, K.~E. and {Wang}, W.-C. and
{Wetherald}, R.~T.},
title = {{Uncertainties in Carbon Dioxide Radiative Forcing in Atmospheric General Circulation Models}},
journal = {Science},
year = 1993,
month = nov,
volume = 262,
pages = {1252-1255},
abstract = {{Global warming, caused by an increase in the concentrations of
greenhouse gases, is the direct result of greenhouse gas-induced
radiative forcing. When a doubling of atmospheric carbon dioxide is
considered, this forcing differed substantially among 15 atmospheric
general circulation models. Although there are several potential causes,
the largest contributor was the carbon dioxide radiation
parameterizations of the models.
}},
doi = {10.1126/science.262.5137.1252},
adsurl = {http://adsabs.harvard.edu/abs/1993Sci...262.1252C},
adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}
@article{1993JGR....9818923N,
author = {{Nesme-Ribes}, E. and {Ferreira}, E.~N. and {Sadourny}, R. and
{Le Treut}, H. and {Li}, Z.~X.},
title = {{Solar dynamics and its impact on solar irradiance and the terrestrial climate}},
journal = {\jgr},
keywords = {Atmospheric General Circulation Models, Climate, Energy Transfer, Irradiance, Solar Activity, Solar Cycles, Solar Terrestrial Interactions, Astrodynamics, Climate Models, Gravitational Fields, Greenhouse Effect, Kinetic Energy, Magnetic Effects, Solar Flux, Stellar Luminosity, Thermal Energy},
year = 1993,
month = nov,
volume = 98,
pages = {18923},
abstract = {{Among the various uncertainties present in climate modeling, the
variability of total solar irradiance is not one of the least. For lack
of any direct measure of the solar irradiance in the past, substitutes
are needed. However, the difficulties are twofold: (1) the reliability
of the proxies and (2) the need for some physical mechanism relating
these proxies to the solar luminosity. On the basis of a better
understanding of the solar machinery we can now propose a plausible
scenario connecting the exchanges of energy between the various
reservoirs: magnetic, thermal, gravitational, and kinetic. In the
present paper we discuss the available proxies and suggest a way to
reconstruct total solar irradiance over the past four centuries. The
response of the Laboratoire de Meteorologie Dynamique atmospheric
general circulation model to magnetoconvective solar forcing during the
Maunder minimum is discussed. The simulated cooling appears to be
compatible with temperature data from the Little Ice Age; in addition,
it is found that variations of globally homogeneous external forcing
parameters, like incoming solar flux or greenhouse gas loading, yield
climate responses with very similar geographical patterns.
}},
doi = {10.1029/93JA00305},
adsurl = {http://adsabs.harvard.edu/abs/1993JGR....9818923N},
adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}
