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Key features of RRTMG_LW are:
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Absorption coefficient data for the k-distributions are obtained directly from the
line-by-line radiative transfer model, LBLRTM,
which has been extensively validated against observations, principally at the
ARM SGP site. Data are consistent with those used in RRTM_LW_v3.0.1, which is
described here.
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Fluxes and heating rates can be calculated over sixteen contiguous bands in the
longwave (10-3250 cm-1, or 3.08-1000 microns). The individual band
ranges (in wavenumbers, cm-1) are: 10-350, 350-500, 500-630,
630-700, 700-820, 820-980, 980-1080, 1080-1180, 1180-1390, 1390-1480, 1480-1800,
1800-2080, 2080-2250, 2250-2380, 2380-2600, and 2600-3250.
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When results are integrated over the full longwave spectrum, the 2600-3250
cm-1 band includes a small adjustment to add the contribution over
the spectral interval from 3250 cm-1 to infinity.
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Modeled molecular absorbers are water vapor, carbon dioxide, ozone,
nitrous oxide, methane, oxygen, nitrogen and several halocarbons (CFC-11,
CFC-12, CFC-22, and CCL4)
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Uses reduced set of g-intervals (140) for integration over absorption in
each band relative to full set of g-intervals used in RRTM_LW (256)
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Includes McICA (Monte-Carlo Independant Column Approximation) capability
to represent sub-grid cloud variability with random, maximum-random,
maximum, exponential, and exponential-random options for cloud overlap;
the exponential and exponential-random methods allow specification of the
required decorrelation length as a constant or as a variable that varies
as a function of latitude and day of the year; References: Barker et al.
(2003); Pincus et al., JGR, (2003); Oreopoulos et al., ACP, (2012)
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Performs radiative transfer for a single (diffusivity) angle (angle = 53 deg;
secant angle = 1.66) and improves accuracy in profiles with high water by
varying the angle in some bands as a function of total column water
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Coding has been reformatted to use many FORTRAN90 features
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Model able to run either as a column model or as a callable subroutine
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Fluxes calculated by RRTMG_LW agree with those computed by LBLRTM within 1.0
W/m2 at all levels, and the computed cooling rates generally agree to within 0.1
K/day in the troposphere and 0.3 K/day in the stratosphere
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Water clouds:
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The optical properties of water clouds are calculated for each spectral
band from the Hu and Stamnes parameterization. The optical depth,
single-scattering albedo, and asymmetry parameter are parameterized as
a function of cloud equivalent radius and liquid water path.
Reference: Hu, Y. X., and K. Stamnes, An accurate parameterization
of the radiative properties of water clouds suitable for use in climate
models. J. Climate, Vol. 6, 728-742, 1993.
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Ice clouds:
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The optical properties of ice clouds are calculated for each spectral band
from the Fu et al. ice particle parameterization.
Reference: Fu, Yang, and Sun, J. Climate,
Vol 11, 1998, pp. 2223-2237, 1998.
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Aerosols:
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Aerosol absorption in the longwave can be included by providing the bulk
aerosol optical depth at the mid-point of each spectral band.
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Absorption coefficients and other initialization data can be optionally input
through a netCDF data file. This feature was developed and provided by
Patrick Hofmann and Robert Pincus of NOAA.
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An optional feature is available to calculate the change in upward flux by
layer as a function of surface temperature. This can be used to approximate
adjustments in upward flux caused only by a change in surface temperature
in a GCM at time intervals between full radiation calls. This is derived
using the pre-calculated derivative of the Planck function with respect to
temperature.
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