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Mesoscale Atmospheric Modeling of Extreme Velocities over the Sea of Okhotsk and Sakhalin

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Abstract

A detailed modeling of meteorological parameters over the last 30 years (1985–2014) has been performed for the Sea of Okhotsk and Sakhalin regions in the frame of the COSMO-CLM regional mesometeorological nonhydrostatic atmospheric model. The downscaling technology is suggested and achieved with three consequent “nesting domains” (with 13.2-, 6.6-, and 2.2-km grid scales). The COSMO-CLM model reproduces (especially successfully on the 2.2-km grid scale) the extremes of wind velocity observed by meteorological stations well. Synoptic situations accompanied by extreme wind speeds are reproduced in detail.

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Correspondence to A. V. Kislov.

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Original Russian Text © A.V. Kislov, G.S. Rivin, V.S. Platonov, M.I. Varentsov, I.A. Rozinkina, M.A. Nikitin, M.M. Chumakov, 2018, published in Izvestiya Rossiiskoi Akademii Nauk, Fizika Atmosfery i Okeana, 2018, Vol. 54, No. 4, pp. 381–385.

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Kislov, A.V., Rivin, G.S., Platonov, V.S. et al. Mesoscale Atmospheric Modeling of Extreme Velocities over the Sea of Okhotsk and Sakhalin. Izv. Atmos. Ocean. Phys. 54, 322–326 (2018). https://doi.org/10.1134/S0001433818040242

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  • DOI: https://doi.org/10.1134/S0001433818040242

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