2006
DOI: 10.1175/jcli3823.1
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Radiative Fluxes in the ECHAM5 General Circulation Model

Abstract: Radiative fluxes in the ECHAM5 general circulation model (GCM) are evaluated using both surface and satellite-based observations. The fluxes at the top of the atmosphere (TOA) are generally in good agreement with the satellite data. Larger deviations in simulated cloud forcing are found especially at lower latitudes where the shortwave component within the intertropical convergence zone is overestimated during boreal summer and underestimated in the marine stratocumulus regimes, especially during boreal winter… Show more

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Cited by 65 publications
(45 citation statements)
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“…Discrepancies between modelled and observed SW and LW cloud forcings suggest that the amount of low clouds may be overestimated in the model (Wild and Roeckner, 2006). It is not clear whether the overestimation involves liquid or ice clouds, or is associated with the cloud cover or the cloud lifetime.…”
Section: Conclusion and Discussionmentioning
confidence: 95%
“…Discrepancies between modelled and observed SW and LW cloud forcings suggest that the amount of low clouds may be overestimated in the model (Wild and Roeckner, 2006). It is not clear whether the overestimation involves liquid or ice clouds, or is associated with the cloud cover or the cloud lifetime.…”
Section: Conclusion and Discussionmentioning
confidence: 95%
“…The tracer advection is calculated with a mass conserving flux form semi-Lagrangian scheme (Lin and Rood, 1996). The ECHAM5 radiation scheme distinguishes four UV-VIS and near-IR, and 16 thermal IR spectral regions (Wild and Roeckner, 2006), and it utilizes the online computed tracer distributions. Photolysis rate calculations for the troposphere up to the mesosphere are based on the eight spectral band approach described in Landgraf and Crutzen (1998), considering absorption and scattering by gases, aerosols and clouds in a delta-two-stream method.…”
Section: Numerical Modelmentioning
confidence: 99%
“…Aspects of the radiation parameterization and its validation are described in Roeckner et al (2003) and Wild and Roeckner (2006), respectively. The standard spectral resolution of the solar radiation parameterization is 4 bands (referenced here as SW4, see Table 1), with 1 band for the UV and visible (250 to 690 nm) and three bands for the near-infrared (690 to 4000 nm).…”
Section: Radiation Parameterizationsmentioning
confidence: 99%