Can we improve the realism of gravity wave parameterizations by imposing sources at all altitudes in the atmosphere?

A multiwave non-orographic gravity waves (GWs) scheme is adapted to represent waves of small intrinsic phase speed, inertial waves, and wave emission from all altitudes. This last change removes the launching altitude parameter, an arbitrary parameter systematically used in GW schemes. In offline ca...

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Detalles Bibliográficos
Autores: Ribstein, Bruno, Millet, Christophe, Lott, François, De La Cámara Illescas, Álvaro
Tipo de recurso: artículo
Fecha de publicación:2022
País:España
Institución:Universidad Complutense de Madrid (UCM)
Repositorio:Docta Complutense
Idioma:inglés
OAI Identifier:oai:docta.ucm.es:20.500.14352/108237
Acceso en línea:https://hdl.handle.net/20.500.14352/108237
Access Level:acceso abierto
Palabra clave:551.51
Gravity waves
Parameterization
Climate model
Middle atmosphere
Física atmosférica
2501 Ciencias de la Atmósfera
Descripción
Sumario:A multiwave non-orographic gravity waves (GWs) scheme is adapted to represent waves of small intrinsic phase speed, inertial waves, and wave emission from all altitudes. This last change removes the launching altitude parameter, an arbitrary parameter systematically used in GW schemes. In offline calculations using reanalysis fields, these changes impose larger amplitude, saturated waves everywhere in the middle atmosphere, which produces more realistic GW vertical spectra than in previous configurations. The same scheme, tested online in the Laboratoire de Météorologie Dynamique Zoom (LMDz) general circulation model, performs at least as well as the operational non-orographic GW scheme. Some modest benefits are seen, for instance, in the equatorial tilt with altitude of the winter jets in the middle atmosphere. Although the scheme includes the effects of inertial waves, which are detected in the mesosphere by different observational platforms, the configuration that gives a reasonable climatology in LMDz hinders their vertical propagation and limits their presence at mesospheric altitudes.