Large-scale anisotropy in stably stratified rotating flows

Autores
Marino, R.; Mininni, Pablo Daniel; Rosenberg, D. L.; Pouquet, A.
Año de publicación
2014
Idioma
inglés
Tipo de recurso
artículo
Estado
versión publicada
Descripción
We present results from direct numerical simulations of the Boussinesq equations in the presence of rotation and/or stratification, both in the vertical direction. The runs are forced isotropically and randomly at small scales and have spatial resolutions of up to 1024 3 grid points and Reynolds numbers of ≈ 1000 . We first show that solutions with negative energy flux and inverse cascades develop in rotating turbulence, whether or not stratification is present. However, the purely stratified case is characterized instead by an early-time, highly anisotropic transfer to large scales with almost zero net isotropic energy flux. This is consistent with previous studies that observed the development of vertically sheared horizontal winds, although only at substantially later times. However, and unlike previous works, when sufficient scale separation is allowed between the forcing scale and the domain size, the kinetic energy displays a perpendicular (horizontal) spectrum with power-law behavior compatible with ∼ k − 5 / 3 ⊥ , including in the absence of rotation. In this latter purely stratified case, such a spectrum is the result of a direct cascade of the energy contained in the large-scale horizontal wind, as is evidenced by a strong positive flux of energy in the parallel direction at all scales including the largest resolved scales.
Fil: Marino, R.. National Center for Atmospheric Research; Estados Unidos. University Of California Berkeley; Estados Unidos
Fil: Mininni, Pablo Daniel. Consejo Nacional de Investigaciones Científicas y Técnicas. Oficina de Coordinación Administrativa Ciudad Universitaria. Instituto de Física de Buenos Aires. Universidad de Buenos Aires. Facultad de Ciencias Exactas y Naturales. Instituto de Física de Buenos Aires; Argentina
Fil: Rosenberg, D. L.. National Center for Computational Sciences; Estados Unidos
Fil: Pouquet, A.. National Center for Atmospheric Research; Estados Unidos. State University Of Colorado Boulder; Estados Unidos
Materia
Stratification
Anisotropic Flows
Turbulence
Boussinesq Flows
Nivel de accesibilidad
acceso abierto
Condiciones de uso
https://creativecommons.org/licenses/by-nc-sa/2.5/ar/
Repositorio
CONICET Digital (CONICET)
Institución
Consejo Nacional de Investigaciones Científicas y Técnicas
OAI Identificador
oai:ri.conicet.gov.ar:11336/18268

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spelling Large-scale anisotropy in stably stratified rotating flowsMarino, R.Mininni, Pablo DanielRosenberg, D. L.Pouquet, A.StratificationAnisotropic FlowsTurbulenceBoussinesq Flowshttps://purl.org/becyt/ford/1.3https://purl.org/becyt/ford/1We present results from direct numerical simulations of the Boussinesq equations in the presence of rotation and/or stratification, both in the vertical direction. The runs are forced isotropically and randomly at small scales and have spatial resolutions of up to 1024 3 grid points and Reynolds numbers of ≈ 1000 . We first show that solutions with negative energy flux and inverse cascades develop in rotating turbulence, whether or not stratification is present. However, the purely stratified case is characterized instead by an early-time, highly anisotropic transfer to large scales with almost zero net isotropic energy flux. This is consistent with previous studies that observed the development of vertically sheared horizontal winds, although only at substantially later times. However, and unlike previous works, when sufficient scale separation is allowed between the forcing scale and the domain size, the kinetic energy displays a perpendicular (horizontal) spectrum with power-law behavior compatible with ∼ k − 5 / 3 ⊥ , including in the absence of rotation. In this latter purely stratified case, such a spectrum is the result of a direct cascade of the energy contained in the large-scale horizontal wind, as is evidenced by a strong positive flux of energy in the parallel direction at all scales including the largest resolved scales.Fil: Marino, R.. National Center for Atmospheric Research; Estados Unidos. University Of California Berkeley; Estados UnidosFil: Mininni, Pablo Daniel. Consejo Nacional de Investigaciones Científicas y Técnicas. Oficina de Coordinación Administrativa Ciudad Universitaria. Instituto de Física de Buenos Aires. Universidad de Buenos Aires. Facultad de Ciencias Exactas y Naturales. Instituto de Física de Buenos Aires; ArgentinaFil: Rosenberg, D. L.. National Center for Computational Sciences; Estados UnidosFil: Pouquet, A.. National Center for Atmospheric Research; Estados Unidos. State University Of Colorado Boulder; Estados UnidosAmerican Physical Society2014-08info:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersionhttp://purl.org/coar/resource_type/c_6501info:ar-repo/semantics/articuloapplication/pdfapplication/pdfhttp://hdl.handle.net/11336/18268Marino, R.; Mininni, Pablo Daniel; Rosenberg, D. L.; Pouquet, A.; Large-scale anisotropy in stably stratified rotating flows; American Physical Society; Physical Review E: Statistical, Nonlinear And Soft Matter Physics; 90; 2; 8-2014; 1-10; 0230181539-3755CONICET DigitalCONICETenginfo:eu-repo/semantics/altIdentifier/doi/10.1103/PhysRevE.90.023018info:eu-repo/semantics/altIdentifier/url/https://journals.aps.org/pre/abstract/10.1103/PhysRevE.90.023018info:eu-repo/semantics/altIdentifier/url/https://arxiv.org/abs/1407.4580info:eu-repo/semantics/openAccesshttps://creativecommons.org/licenses/by-nc-sa/2.5/ar/reponame:CONICET Digital (CONICET)instname:Consejo Nacional de Investigaciones Científicas y Técnicas2025-09-03T09:54:43Zoai:ri.conicet.gov.ar:11336/18268instacron:CONICETInstitucionalhttp://ri.conicet.gov.ar/Organismo científico-tecnológicoNo correspondehttp://ri.conicet.gov.ar/oai/requestdasensio@conicet.gov.ar; lcarlino@conicet.gov.arArgentinaNo correspondeNo correspondeNo correspondeopendoar:34982025-09-03 09:54:43.657CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicasfalse
dc.title.none.fl_str_mv Large-scale anisotropy in stably stratified rotating flows
title Large-scale anisotropy in stably stratified rotating flows
spellingShingle Large-scale anisotropy in stably stratified rotating flows
Marino, R.
Stratification
Anisotropic Flows
Turbulence
Boussinesq Flows
title_short Large-scale anisotropy in stably stratified rotating flows
title_full Large-scale anisotropy in stably stratified rotating flows
title_fullStr Large-scale anisotropy in stably stratified rotating flows
title_full_unstemmed Large-scale anisotropy in stably stratified rotating flows
title_sort Large-scale anisotropy in stably stratified rotating flows
dc.creator.none.fl_str_mv Marino, R.
Mininni, Pablo Daniel
Rosenberg, D. L.
Pouquet, A.
author Marino, R.
author_facet Marino, R.
Mininni, Pablo Daniel
Rosenberg, D. L.
Pouquet, A.
author_role author
author2 Mininni, Pablo Daniel
Rosenberg, D. L.
Pouquet, A.
author2_role author
author
author
dc.subject.none.fl_str_mv Stratification
Anisotropic Flows
Turbulence
Boussinesq Flows
topic Stratification
Anisotropic Flows
Turbulence
Boussinesq Flows
purl_subject.fl_str_mv https://purl.org/becyt/ford/1.3
https://purl.org/becyt/ford/1
dc.description.none.fl_txt_mv We present results from direct numerical simulations of the Boussinesq equations in the presence of rotation and/or stratification, both in the vertical direction. The runs are forced isotropically and randomly at small scales and have spatial resolutions of up to 1024 3 grid points and Reynolds numbers of ≈ 1000 . We first show that solutions with negative energy flux and inverse cascades develop in rotating turbulence, whether or not stratification is present. However, the purely stratified case is characterized instead by an early-time, highly anisotropic transfer to large scales with almost zero net isotropic energy flux. This is consistent with previous studies that observed the development of vertically sheared horizontal winds, although only at substantially later times. However, and unlike previous works, when sufficient scale separation is allowed between the forcing scale and the domain size, the kinetic energy displays a perpendicular (horizontal) spectrum with power-law behavior compatible with ∼ k − 5 / 3 ⊥ , including in the absence of rotation. In this latter purely stratified case, such a spectrum is the result of a direct cascade of the energy contained in the large-scale horizontal wind, as is evidenced by a strong positive flux of energy in the parallel direction at all scales including the largest resolved scales.
Fil: Marino, R.. National Center for Atmospheric Research; Estados Unidos. University Of California Berkeley; Estados Unidos
Fil: Mininni, Pablo Daniel. Consejo Nacional de Investigaciones Científicas y Técnicas. Oficina de Coordinación Administrativa Ciudad Universitaria. Instituto de Física de Buenos Aires. Universidad de Buenos Aires. Facultad de Ciencias Exactas y Naturales. Instituto de Física de Buenos Aires; Argentina
Fil: Rosenberg, D. L.. National Center for Computational Sciences; Estados Unidos
Fil: Pouquet, A.. National Center for Atmospheric Research; Estados Unidos. State University Of Colorado Boulder; Estados Unidos
description We present results from direct numerical simulations of the Boussinesq equations in the presence of rotation and/or stratification, both in the vertical direction. The runs are forced isotropically and randomly at small scales and have spatial resolutions of up to 1024 3 grid points and Reynolds numbers of ≈ 1000 . We first show that solutions with negative energy flux and inverse cascades develop in rotating turbulence, whether or not stratification is present. However, the purely stratified case is characterized instead by an early-time, highly anisotropic transfer to large scales with almost zero net isotropic energy flux. This is consistent with previous studies that observed the development of vertically sheared horizontal winds, although only at substantially later times. However, and unlike previous works, when sufficient scale separation is allowed between the forcing scale and the domain size, the kinetic energy displays a perpendicular (horizontal) spectrum with power-law behavior compatible with ∼ k − 5 / 3 ⊥ , including in the absence of rotation. In this latter purely stratified case, such a spectrum is the result of a direct cascade of the energy contained in the large-scale horizontal wind, as is evidenced by a strong positive flux of energy in the parallel direction at all scales including the largest resolved scales.
publishDate 2014
dc.date.none.fl_str_mv 2014-08
dc.type.none.fl_str_mv info:eu-repo/semantics/article
info:eu-repo/semantics/publishedVersion
http://purl.org/coar/resource_type/c_6501
info:ar-repo/semantics/articulo
format article
status_str publishedVersion
dc.identifier.none.fl_str_mv http://hdl.handle.net/11336/18268
Marino, R.; Mininni, Pablo Daniel; Rosenberg, D. L.; Pouquet, A.; Large-scale anisotropy in stably stratified rotating flows; American Physical Society; Physical Review E: Statistical, Nonlinear And Soft Matter Physics; 90; 2; 8-2014; 1-10; 023018
1539-3755
CONICET Digital
CONICET
url http://hdl.handle.net/11336/18268
identifier_str_mv Marino, R.; Mininni, Pablo Daniel; Rosenberg, D. L.; Pouquet, A.; Large-scale anisotropy in stably stratified rotating flows; American Physical Society; Physical Review E: Statistical, Nonlinear And Soft Matter Physics; 90; 2; 8-2014; 1-10; 023018
1539-3755
CONICET Digital
CONICET
dc.language.none.fl_str_mv eng
language eng
dc.relation.none.fl_str_mv info:eu-repo/semantics/altIdentifier/doi/10.1103/PhysRevE.90.023018
info:eu-repo/semantics/altIdentifier/url/https://journals.aps.org/pre/abstract/10.1103/PhysRevE.90.023018
info:eu-repo/semantics/altIdentifier/url/https://arxiv.org/abs/1407.4580
dc.rights.none.fl_str_mv info:eu-repo/semantics/openAccess
https://creativecommons.org/licenses/by-nc-sa/2.5/ar/
eu_rights_str_mv openAccess
rights_invalid_str_mv https://creativecommons.org/licenses/by-nc-sa/2.5/ar/
dc.format.none.fl_str_mv application/pdf
application/pdf
dc.publisher.none.fl_str_mv American Physical Society
publisher.none.fl_str_mv American Physical Society
dc.source.none.fl_str_mv reponame:CONICET Digital (CONICET)
instname:Consejo Nacional de Investigaciones Científicas y Técnicas
reponame_str CONICET Digital (CONICET)
collection CONICET Digital (CONICET)
instname_str Consejo Nacional de Investigaciones Científicas y Técnicas
repository.name.fl_str_mv CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicas
repository.mail.fl_str_mv dasensio@conicet.gov.ar; lcarlino@conicet.gov.ar
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