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The growing field of exoplanetary atmospheric modelling has seen little workon standardised benchmark tests for its models, limiting understanding of thedependence of results on specific models and conditions. With spatiallyresolved observations as yet difficult to obtain, such a test is invaluable.Although an intercomparison test for models of tidally locked gas giant planetshas previously been suggested and carried out, the data provided were limitedin terms of comparability. Here, the shallow PUMA model is subjected to such atest, and detailed statistics produced to facilitate comparison, with both timemeans and the associated standard deviations displayed, removing the timedependence and providing a measure of the variability. Model runs have beenanalysed to determine the variability between resolutions, and the effect ofresolution on the energy spectra studied. Superrotation is a robust andreproducible feature at all resolutions.

Benchmark experiments with global climate models applicable to extra-solar gas giant planets in the shallow atmosphere approximation