Emergence of helicity in rotating stratified turbulence

• Autores: Marino, Raffaele; Mininni, Pablo Daniel; Rosenberg, Duane; Pouquet, Annick
• Año de publicación: 2013
• Idioma: inglés
• Tipo de recurso: artículo
• Materia: ROTATING FLOWS; STRATIFIED FLOWS; HELICITY; GEOSTROPHY
• Institución: Consejo Nacional de Investigaciones Científicas y Técnicas

We perform numerical simulations of decaying rotating stratified turbulence and show, in the Boussinesq framework, that helicity (velocity-vorticity correlation), as observed in supercell storms and hurricanes, is spontaneously created due to an interplay between buoyancy and rotation common to large-scale atmospheric and oceanic flows. Helicity emerges from the joint action of eddies and of inertia-gravity waves (with inertia and gravity with respective associated frequencies f and N), and it occurs when the waves are sufficiently strong. For N/ f <3 the amount of helicity produced is correctly predicted by a quasilinear balance equation. Outside this regime, and up to the highest Reynolds number obtained in this study, namely Re≈10 000, helicity production is found to be persistent forN/f as large as ≈17, and for ReFr 2 and ReRo 2, respectively, as large as ≈100 and ≈24000.
Fil: Marino, Raffaele. National Center for Atmospheric Research; Estados Unidos de América;
Fil: Mininni, Pablo Daniel. Consejo Nacional de Investigaciones Científicas y Técnicas. Oficina de Coordinación Administrativa Ciudad Universitaria. Instituto de Física de Buenos Aires; Argentina;
Fil: Rosenberg, Duane. National Center for Computational Sciences. Oak Ridge National Laboratory; Estados Unidos de América;
Fil: Pouquet, Annick. Department of Applied Mathematics. University of Colorado at Boulder; Estados Unidos de América;