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In the context of the MOSE project, in this contribution we present adetailed analysis of the Meso-NH mesoscale model performances and theirdependency on the model and orography horizontal resolutions in proximity ofthe ground. The investigated sites are Cerro Paranal (site of the ESO VeryLarge Telescope - VLT) and Cerro Armazones (site of the ESO European ExtremelyLarge Telescope - E-ELT), in Chile. At both sites, data from a rich statisticalsample of different nights are available - from AWS (Automated WeatherStations) and masts - giving access to wind speed, wind direction andtemperature at different levels near the ground (from 2 m to 30 m above theground). In this study we discuss the use of a very high horizontal resolution(dX=0.1 km) numerical configuration that overcomes some specific limitationsput in evidence with a standard configuration with dX=0.5 km. In both sitesresults are very promising. The study is co-funded by ESO and INAF.

MOSE: zooming on the Meso-NH mesoscale model performances at the surface layer at ESO sites (Paranal and Armazones)