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Análisis del evento supercelular del 31 de julio de 2015 en España con el modelo WRF-ARW.

  • Díaz-Fernández, Javier [1] ; Calvo-Sancho, Carlos [2] ; Quitián-Hernández, Lara [2] ; Bolgiani, Pedro [1] ; Santos-Muñoz, Daniel [4] Árbol académico ; Luna Rico, María Yolanda [3] ; González-Alemán, Juan Jesús [3] Árbol académico ; Sastre, Mariano [1] ; Valero, Francisco [1] Árbol académico ; Farrán, José Ignacio [2] ; Martín, María Luisa [2] Árbol académico
    1. [1] Universidad Complutense de Madrid

      Universidad Complutense de Madrid

      Madrid, España

    2. [2] Universidad de Valladolid

      Universidad de Valladolid

      Valladolid, España

    3. [3] Agencia Estatal de Meteorología

      Agencia Estatal de Meteorología

      Madrid, España

    4. [4] Instituto Danés de Meteorología. Copenhague.
  • Localización: 10.ª Asamblea Hispano-Portuguesa de Geodesia y Geofísica: artículos, 2023, ISBN 978-84-416-7540-7, págs. 791-796
  • Idioma: español
  • Títulos paralelos:
    • Analysis of the supercell event of 31 July 2015 in Spain with the WRF-ARW model.
  • Enlaces
  • Resumen
    • Supercells are a type of severe convective storms usually associated with adverse meteorological phenomena (large hail, strong winds, thunderstorms, floods, tornadoes...). These phenomena can be extremely destructive and cause a great deal of material damage and occasionally personal injuries. Therefore, it is important to study supercells in detail to achieve a correct forecast and anticipate possible consequences. In this paper, a supercell event occurred in eastern Spain on 31 July 2015 is presented. The event caused great destruction in several locations due to strong winds and large hail (greater than 8 cm diameter). The system was simulated with the Weather Research and Forecasting (WRF-ARW) model. The synoptic situation was characterized by the presence of a deep trough whose axis was located over the Iberian Peninsula, promoting positive vorticity and divergence advection to occur in front of the axis, providing a favorable convective environment for the supercells development. The MSG-SEVIRI satellite brightness temperature (10.8 µm infrared channel) is used as a meteorological variable to validate and compare the simulations of the cloudiness associated with the supercell event. The validation of the WRF model is performed thorough several skill-scores, giving satisfactory results in the distribution of the brightness temperature of the supercells with a slight overestimation of it.

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