The availability of this unique dataset provides a valuable opportunity to evaluate the ability of a particular physical parameterization suite to accurately simulate the atmospheric state for a diverse range of cloud types and conditions. Thus far, synthetic SEVIRI infrared brightness temperatures and CloudSat cloud reflectivities have been computed for this case. Preliminary comparisons between the real and simulated observations are very encouraging. For instance, probability distributions constructed for each SEVIRI channel show a remarkable level of agreement with mean brightness temperature biases generally less than 1 K over the entire model domain. Although limited in geographical coverage, CloudSat observations were used to examine the vertical structure of the simulated cloud fields. Overall, the simulation realistically depicted the vertical structure of many cloud types, particularly those associated with mid-latitude disturbances, but performed poorly in other regions, such as those containing shallow marine stratocumulus clouds.
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