Simulation of Atmospheric Microbursts Using a Numerical Mesoscale Model at High Spatiotemporal Resolution
[EN] Atmospheric microbursts are low-level meteorological events that can produce significant damage on the surface and pose a major risk to aircraft flying close to the ground. Studies and ad hoc numerical models have been developed to understand the origin and dynamics of the microburst; neverthel...
| Autores: | , , , , , , |
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| Tipo de recurso: | artículo |
| Estado: | Versión publicada |
| Fecha de publicación: | 2020 |
| País: | España |
| Institución: | Universidad de León |
| Repositorio: | BULERIA. Repositorio Institucional de la Universidad de León |
| OAI Identifier: | oai:buleria.unileon.es:10612/24789 |
| Acceso en línea: | https://agupubs.onlinelibrary.wiley.com/doi/10.1029/2019JD031791 https://hdl.handle.net/10612/24789 |
| Access Level: | acceso abierto |
| Palabra clave: | Física Meteorología Deep convection Downburst High-reflectivity microburst High resolution Numerical simulation WRF 2509.08 Micrometeorología 2501.21 Simulación Numérica 2509.09 Predicción Numérica Meteorológica 2501.11 Termodinámica Atmosférica |
| Sumario: | [EN] Atmospheric microbursts are low-level meteorological events that can produce significant damage on the surface and pose a major risk to aircraft flying close to the ground. Studies and ad hoc numerical models have been developed to understand the origin and dynamics of the microburst; nevertheless, there are few researches of the phenomenon using global and mesoscale models. This is mainly due to the limitations in resolution, as microbursts normally span for less than 4 km and 20 min. In this paper, the Weather Research and Forecasting model is used at resolutions of 400 m and 3 min to test if it can properly capture the variables and dynamics of high-reflectivity microbursts. Several microphysics and planetary boundary layer parametrizations are tested to find the best model configuration for the simulation of this kind of episodes. General conditions are evaluated by using thermodynamic diagrams. Surface and vertical wind speed, reflectivity, precipitation, and other variables for each simulated event are compared with observations, and the model's sensitivity to the variables is assessed. The dynamics and evolution of the microburst is evaluated using different plots of a chosen event. The results show that the model is able to reproduce high-reflectivity microbursts in accordance with observations, although there is a tendency to underestimate the intensity of variables, most markedly on the wind vertical velocity. Regarding the microphysics schemes, the Morrison parametrization performs better than the WRF single-moment 6-class scheme. No major differences are found between the Mellor-Yamada-Janjic and the Mellor-Yamada-Nakanishi-Niino planetary boundary layer parametrizations |
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