The interplay between helicity and rotation in turbulence: Implications for scaling laws and small-scale dynamics

Autores
Pouquet, A.; Mininni, P.D.
Año de publicación
2010
Idioma
inglés
Tipo de recurso
artículo
Estado
versión publicada
Descripción
Invariance properties of physical systems govern their behaviour: energy conservation in turbulence drives a wide distribution of energy among modes, as observed in geophysical or astrophysical flows. In ideal hydrodynamics, the role of the invariance of helicity (correlation between velocity and its curl, measuring departures from mirror symmetry) remains unclear since it does not alter the energy spectrum. However, in the presence of rotation, significant differences emerge between helical and non-helical turbulent flows. We first briefly outline some of the issues such as the partition of energy and helicity among modes. Using massive numerical simulations, we then show that smallscale structures and their intermittency properties differ according to whether helicity is present or not, in particular with respect to the emergence of Beltrami core vortices that are laminar helical vertical updraft vortices. These results point to the discovery of a small parameter besides the Rossby number, a fact that would relate the problem of rotating helical turbulence to that of critical phenomena, through the renormalization group and weak-turbulence theory. This parameter can be associated with the adimensionalized ratio of the energy to helicity flux to small scales, the three-dimensional energy cascade being weak and self-similar. copy; 2010 The Royal Society.
Fil:Mininni, P.D. Universidad de Buenos Aires. Facultad de Ciencias Exactas y Naturales; Argentina.
Fuente
Philos. Trans. R. Soc. A Math. Phys. Eng. Sci. 2010;368(1916):1635-1662
Materia
Helicity
Intermittency
Scaling laws
Structures
Turbulence
Universality
Computer simulation
Rotation
Scaling laws
Spectroscopy
Statistical mechanics
Astrophysical flows
Beltrami
Critical phenomenon
Energy spectra
Helical turbulence
Helicities
Intermittency
Mirror symmetry
Numerical simulation
Physical systems
Renormalization group
Rossby numbers
Royal society
Self-similar
Small scale
Small-scale dynamics
Small-scale structures
Three-dimensional energy
Turbulence theory
Turbulence
Nivel de accesibilidad
acceso abierto
Condiciones de uso
http://creativecommons.org/licenses/by/2.5/ar
Repositorio
Biblioteca Digital (UBA-FCEN)
Institución
Universidad Nacional de Buenos Aires. Facultad de Ciencias Exactas y Naturales
OAI Identificador
paperaa:paper_1364503X_v368_n1916_p1635_Pouquet

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oai_identifier_str paperaa:paper_1364503X_v368_n1916_p1635_Pouquet
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repository_id_str 1896
network_name_str Biblioteca Digital (UBA-FCEN)
spelling The interplay between helicity and rotation in turbulence: Implications for scaling laws and small-scale dynamicsPouquet, A.Mininni, P.D.HelicityIntermittencyScaling lawsStructuresTurbulenceUniversalityComputer simulationRotationScaling lawsSpectroscopyStatistical mechanicsAstrophysical flowsBeltramiCritical phenomenonEnergy spectraHelical turbulenceHelicitiesIntermittencyMirror symmetryNumerical simulationPhysical systemsRenormalization groupRossby numbersRoyal societySelf-similarSmall scaleSmall-scale dynamicsSmall-scale structuresThree-dimensional energyTurbulence theoryTurbulenceInvariance properties of physical systems govern their behaviour: energy conservation in turbulence drives a wide distribution of energy among modes, as observed in geophysical or astrophysical flows. In ideal hydrodynamics, the role of the invariance of helicity (correlation between velocity and its curl, measuring departures from mirror symmetry) remains unclear since it does not alter the energy spectrum. However, in the presence of rotation, significant differences emerge between helical and non-helical turbulent flows. We first briefly outline some of the issues such as the partition of energy and helicity among modes. Using massive numerical simulations, we then show that smallscale structures and their intermittency properties differ according to whether helicity is present or not, in particular with respect to the emergence of Beltrami core vortices that are laminar helical vertical updraft vortices. These results point to the discovery of a small parameter besides the Rossby number, a fact that would relate the problem of rotating helical turbulence to that of critical phenomena, through the renormalization group and weak-turbulence theory. This parameter can be associated with the adimensionalized ratio of the energy to helicity flux to small scales, the three-dimensional energy cascade being weak and self-similar. copy; 2010 The Royal Society.Fil:Mininni, P.D. Universidad de Buenos Aires. Facultad de Ciencias Exactas y Naturales; Argentina.2010info:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersionhttp://purl.org/coar/resource_type/c_6501info:ar-repo/semantics/articuloapplication/pdfhttp://hdl.handle.net/20.500.12110/paper_1364503X_v368_n1916_p1635_PouquetPhilos. Trans. R. Soc. A Math. Phys. Eng. Sci. 2010;368(1916):1635-1662reponame:Biblioteca Digital (UBA-FCEN)instname:Universidad Nacional de Buenos Aires. Facultad de Ciencias Exactas y Naturalesinstacron:UBA-FCENenginfo:eu-repo/semantics/openAccesshttp://creativecommons.org/licenses/by/2.5/ar2025-10-16T09:30:20Zpaperaa:paper_1364503X_v368_n1916_p1635_PouquetInstitucionalhttps://digital.bl.fcen.uba.ar/Universidad públicaNo correspondehttps://digital.bl.fcen.uba.ar/cgi-bin/oaiserver.cgiana@bl.fcen.uba.arArgentinaNo correspondeNo correspondeNo correspondeopendoar:18962025-10-16 09:30:22.882Biblioteca Digital (UBA-FCEN) - Universidad Nacional de Buenos Aires. Facultad de Ciencias Exactas y Naturalesfalse
dc.title.none.fl_str_mv The interplay between helicity and rotation in turbulence: Implications for scaling laws and small-scale dynamics
title The interplay between helicity and rotation in turbulence: Implications for scaling laws and small-scale dynamics
spellingShingle The interplay between helicity and rotation in turbulence: Implications for scaling laws and small-scale dynamics
Pouquet, A.
Helicity
Intermittency
Scaling laws
Structures
Turbulence
Universality
Computer simulation
Rotation
Scaling laws
Spectroscopy
Statistical mechanics
Astrophysical flows
Beltrami
Critical phenomenon
Energy spectra
Helical turbulence
Helicities
Intermittency
Mirror symmetry
Numerical simulation
Physical systems
Renormalization group
Rossby numbers
Royal society
Self-similar
Small scale
Small-scale dynamics
Small-scale structures
Three-dimensional energy
Turbulence theory
Turbulence
title_short The interplay between helicity and rotation in turbulence: Implications for scaling laws and small-scale dynamics
title_full The interplay between helicity and rotation in turbulence: Implications for scaling laws and small-scale dynamics
title_fullStr The interplay between helicity and rotation in turbulence: Implications for scaling laws and small-scale dynamics
title_full_unstemmed The interplay between helicity and rotation in turbulence: Implications for scaling laws and small-scale dynamics
title_sort The interplay between helicity and rotation in turbulence: Implications for scaling laws and small-scale dynamics
dc.creator.none.fl_str_mv Pouquet, A.
Mininni, P.D.
author Pouquet, A.
author_facet Pouquet, A.
Mininni, P.D.
author_role author
author2 Mininni, P.D.
author2_role author
dc.subject.none.fl_str_mv Helicity
Intermittency
Scaling laws
Structures
Turbulence
Universality
Computer simulation
Rotation
Scaling laws
Spectroscopy
Statistical mechanics
Astrophysical flows
Beltrami
Critical phenomenon
Energy spectra
Helical turbulence
Helicities
Intermittency
Mirror symmetry
Numerical simulation
Physical systems
Renormalization group
Rossby numbers
Royal society
Self-similar
Small scale
Small-scale dynamics
Small-scale structures
Three-dimensional energy
Turbulence theory
Turbulence
topic Helicity
Intermittency
Scaling laws
Structures
Turbulence
Universality
Computer simulation
Rotation
Scaling laws
Spectroscopy
Statistical mechanics
Astrophysical flows
Beltrami
Critical phenomenon
Energy spectra
Helical turbulence
Helicities
Intermittency
Mirror symmetry
Numerical simulation
Physical systems
Renormalization group
Rossby numbers
Royal society
Self-similar
Small scale
Small-scale dynamics
Small-scale structures
Three-dimensional energy
Turbulence theory
Turbulence
dc.description.none.fl_txt_mv Invariance properties of physical systems govern their behaviour: energy conservation in turbulence drives a wide distribution of energy among modes, as observed in geophysical or astrophysical flows. In ideal hydrodynamics, the role of the invariance of helicity (correlation between velocity and its curl, measuring departures from mirror symmetry) remains unclear since it does not alter the energy spectrum. However, in the presence of rotation, significant differences emerge between helical and non-helical turbulent flows. We first briefly outline some of the issues such as the partition of energy and helicity among modes. Using massive numerical simulations, we then show that smallscale structures and their intermittency properties differ according to whether helicity is present or not, in particular with respect to the emergence of Beltrami core vortices that are laminar helical vertical updraft vortices. These results point to the discovery of a small parameter besides the Rossby number, a fact that would relate the problem of rotating helical turbulence to that of critical phenomena, through the renormalization group and weak-turbulence theory. This parameter can be associated with the adimensionalized ratio of the energy to helicity flux to small scales, the three-dimensional energy cascade being weak and self-similar. copy; 2010 The Royal Society.
Fil:Mininni, P.D. Universidad de Buenos Aires. Facultad de Ciencias Exactas y Naturales; Argentina.
description Invariance properties of physical systems govern their behaviour: energy conservation in turbulence drives a wide distribution of energy among modes, as observed in geophysical or astrophysical flows. In ideal hydrodynamics, the role of the invariance of helicity (correlation between velocity and its curl, measuring departures from mirror symmetry) remains unclear since it does not alter the energy spectrum. However, in the presence of rotation, significant differences emerge between helical and non-helical turbulent flows. We first briefly outline some of the issues such as the partition of energy and helicity among modes. Using massive numerical simulations, we then show that smallscale structures and their intermittency properties differ according to whether helicity is present or not, in particular with respect to the emergence of Beltrami core vortices that are laminar helical vertical updraft vortices. These results point to the discovery of a small parameter besides the Rossby number, a fact that would relate the problem of rotating helical turbulence to that of critical phenomena, through the renormalization group and weak-turbulence theory. This parameter can be associated with the adimensionalized ratio of the energy to helicity flux to small scales, the three-dimensional energy cascade being weak and self-similar. copy; 2010 The Royal Society.
publishDate 2010
dc.date.none.fl_str_mv 2010
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/20.500.12110/paper_1364503X_v368_n1916_p1635_Pouquet
url http://hdl.handle.net/20.500.12110/paper_1364503X_v368_n1916_p1635_Pouquet
dc.language.none.fl_str_mv eng
language eng
dc.rights.none.fl_str_mv info:eu-repo/semantics/openAccess
http://creativecommons.org/licenses/by/2.5/ar
eu_rights_str_mv openAccess
rights_invalid_str_mv http://creativecommons.org/licenses/by/2.5/ar
dc.format.none.fl_str_mv application/pdf
dc.source.none.fl_str_mv Philos. Trans. R. Soc. A Math. Phys. Eng. Sci. 2010;368(1916):1635-1662
reponame:Biblioteca Digital (UBA-FCEN)
instname:Universidad Nacional de Buenos Aires. Facultad de Ciencias Exactas y Naturales
instacron:UBA-FCEN
reponame_str Biblioteca Digital (UBA-FCEN)
collection Biblioteca Digital (UBA-FCEN)
instname_str Universidad Nacional de Buenos Aires. Facultad de Ciencias Exactas y Naturales
instacron_str UBA-FCEN
institution UBA-FCEN
repository.name.fl_str_mv Biblioteca Digital (UBA-FCEN) - Universidad Nacional de Buenos Aires. Facultad de Ciencias Exactas y Naturales
repository.mail.fl_str_mv ana@bl.fcen.uba.ar
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