Intercomparison of three microwave/infrared high resolution line-by-line radiative transfer codes
Author(s) -
Franz Schreier,
Sebastián Gimeno Garcìa,
M. Milz,
Ajil Kottayil,
M. Höpfner,
T. von Clarmann,
G. P. Stiller
Publication year - 2013
Publication title -
aip conference proceedings
Language(s) - English
Resource type - Conference proceedings
eISSN - 1551-7616
pISSN - 0094-243X
DOI - 10.1063/1.4804722
Subject(s) - depth sounding , infrared , remote sensing , radiative transfer , microwave , nadir , advanced microwave sounding unit , line (geometry) , atmospheric sounding , radiometry , environmental science , physics , optics , satellite , geology , oceanography , geometry , mathematics , quantum mechanics , astronomy
An intercomparison of three line-by-line (lbl) codes developed independently for atmospheric radiative transfer and remote sensing — ARTS, GARLIC, and KOPRA — has been performed for a thermal infrared nadir sounding application assuming a HIRS-like (High resolution Infrared Radiation Sounder) setup. Radiances for the 19 HIRS infrared channels and a set of 42 atmospheric profiles from the “Garand dataset” have been computed. The mutual differences of the equivalent brightness temperatures are presented and possible causes of disagreement are discussed. In particular, the impact of path integration schemes and atmospheric layer discretization is assessed. When the continuum absorption contribution is ignored because of the different implementations, residuals are generally in the sub-Kelvin range and smaller than 0.1 K for some window channels (and all atmospheric models and lbl codes). None of the three codes turned out to be perfect for all channels and atmospheres. Remaining discrepancies are attributed to different lbl optimization techniques. Lbl codes seem to have reached a maturity in the implementation of radiative transfer that the choice of the underlying physical models (line shape models, continua etc) becomes increasingly relevant.
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