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Rapid radiative transfer model

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This is an old revision of this page, as edited by Rjhogan (talk | contribs) at 21:56, 22 October 2017 (Removed links to missing/inappropriate pages; changed shortwave/longwave to solar/thermal-infrared; added a little more detail). The present address (URL) is a permanent link to this revision, which may differ significantly from the current revision.

The Rapid Radiative Transfer Model (RRTM) is a validated, correlated k-distribution band model for the calculation of solar and thermal-infrared atmospheric radiative fluxes and heating rates. The Rapid Radiative Transfer Model for GCMs (RRTM-G) is an accelerated version of RRTM that provides improved efficiency with minimal loss of accuracy for application to general circulation models. The latter divides the solar spectrum into 14 bands within which a total of 112 pseudo-monochromatic calculations are performed, and in the thermal infrared 16 bands are used within which 140 pseudo-monochromatic calculations are performed. RRTM-G is used in a number of general circulation models worldwide, such as that of the European Centre for Medium-Range Weather Forecasts[1].

See also

References

  1. ^ Hogan, Robin J.; Bozzo, Alessio. "ECRAD: A new radiation scheme for the IFS". Retrieved 2017-10-22.
  • Clough, S. A., M. W. Shephard, E. J. Mlawer, J. S. Delamere, M. J. Iacono, K. Cady-Pereira, S. Boukabara, and P. D. Brown, Atmospheric radiative transfer modeling: a summary of the AER codes, Short Communication, J. Quant. Spectrosc. Radiat. Transfer, 91, 233-244, 2005.
  • Mlawer, E.J., S.J. Taubman, P.D. Brown, M.J. Iacono and S.A. Clough: RRTM, a validated correlated-k model for the longwave. J. Geophys. Res., 102, 16,663-16,682, 1997.