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Volkmar Wirth, Michael Riemer, Edmund K. M. Chang, and Olivia Martius

-00304.1 Charney , J. , 1955 : The use of the primitive equations of motion in numerical prediction . Tellus , 7 , 22 – 26 , https://doi.org/10.3402/tellusa.v7i1.8772 . 10.3402/tellusa.v7i1.8772 Charney , J. , and P. G. Drazin , 1961 : Propagation of planetary-scale disturbances from the lower into the upper atmosphere . J. Geophys. Res. , 66 , 83 – 109 , https://doi.org/10.1029/JZ066i001p00083 . 10.1029/JZ066i001p00083 Chen , G. , J. Lu , D. A. Burrows , and L. R. Leung , 2015

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Hilke S. Lentink, Christian M. Grams, Michael Riemer, and Sarah C. Jones

) and http://www.cosmo-model.org for more details on the computational methods]. The model is set up with a horizontal resolution of 0.025° (about 2.5 km at 35°N) and 57 vertical levels up to 30-km height, with an enhanced vertical resolution in the planetary boundary layer. Shallow convection is parameterized using the mass-flux scheme of Tiedtke (1989) , while middle and high convection are explicitly computed. For all parameterized processes, the default setup of COSMO is used ( Doms et al

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