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
- Institución
- Consejo Nacional de Investigaciones Científicas y Técnicas
- OAI Identificador
- oai:ri.conicet.gov.ar:11336/18268
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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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13.13397 |