dc.creatorMininni, Pablo Daniel
dc.creatorPouquet, A.
dc.date.accessioned2018-09-24T18:02:59Z
dc.date.available2018-09-24T18:02:59Z
dc.date.created2018-09-24T18:02:59Z
dc.date.issued2009-12
dc.identifierMininni, Pablo Daniel; Pouquet, A.; Helicity cascades in rotating turbulence; American Physical Society; Physical Review E: Statistical, Nonlinear and Soft Matter Physics; 79; 2; 12-2009; 263041-263047
dc.identifier1539-3755
dc.identifierhttp://hdl.handle.net/11336/60768
dc.identifierCONICET Digital
dc.identifierCONICET
dc.description.abstractThe effect of helicity (velocity-vorticity correlations) is studied in direct numerical simulations of rotating turbulence down to Rossby numbers of 0.02. The results suggest that the presence of net helicity plays an important role in the dynamics of the flow. In particular, at small Rossby number, the energy cascades to large scales, as expected, but helicity then can dominate the cascade to small scales. A phenomenological interpretation in terms of a direct cascade of helicity slowed down by wave-eddy interactions leads to the prediction of non-Kolmogorovian inertial indices for the small-scale energy and helicity spectra. © 2009 The American Physical Society.
dc.languageeng
dc.publisherAmerican Physical Society
dc.relationinfo:eu-repo/semantics/altIdentifier/doi/http://dx.doi.org/10.1103/PhysRevE.79.026304
dc.rightshttps://creativecommons.org/licenses/by-nc-sa/2.5/ar/
dc.rightsinfo:eu-repo/semantics/openAccess
dc.subjectTurbulence
dc.subjectHelicity
dc.titleHelicity cascades in rotating turbulence
dc.typeinfo:eu-repo/semantics/article
dc.typeinfo:ar-repo/semantics/artículo
dc.typeinfo:eu-repo/semantics/publishedVersion


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