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Evolution of spectroscopic information over the last decade and its effect on line-by-line calculations for validation of radiation codes for climate models
Authors:B.A Fomin  T.A Udalova  E.A Zhitnitskii
Affiliation:Russian Research Center, Kurchatov Institute, 1 Kurchatov sq., 123182 Moscow, Russia
Abstract:Five HITRAN's editions (since 1992) and three radically new H2O spectral databases have been tested for their usefulness in line-by-line benchmark calculations for radiation code validations. The longwave calculations for the mid-latitude summer (MLS) atmosphere with the different HITRAN's editions revealed a good convergence (maximal discrepancies since View the MathML source decreased to View the MathML source in our flux calculations with 1992-2002 and 1996-2002 HITRAN's editions, respectively). The shortwave calculations with different HITRAN's editions revealed a good agreement: discrepancies in downward fluxes absorbed by the MLS atmosphere are less than View the MathML source, i.e. 0.5% for the all HITRAN's editions since 1992. It has been determined that it is unreasonable to replace HITRAN by any new H2O spectral database in benchmark calculations, although they contain essentially more spectral lines than HITRAN (up to ∼10 times). Moreover, it has been found that no new database could be useful for explaining the “anomalous absorption” problem. Two latest water vapor continuum models have been tested as well. It has been found out that these models are the main source of uncertainties in the present and previous calculations: discrepancies for the MLS atmosphere reached ∼3 and View the MathML source in the longwave and shortwave flux calculations, respectively.
Keywords:Spectroscopic databases   Continuum models   Atmospheric radiation   Line-by-line calculations   Codes in climate models
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