Large-scale anisotropy in stably stratified rotating flows

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 10243 grid points and Reynolds numb...

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Autores principales: Marino, R., Mininni, P.D., Rosenberg, D.L., Pouquet, A.
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Acceso en línea:http://hdl.handle.net/20.500.12110/paper_15393755_v90_n2_p_Marino
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spelling todo:paper_15393755_v90_n2_p_Marino2023-10-03T16:22:49Z Large-scale anisotropy in stably stratified rotating flows Marino, R. Mininni, P.D. Rosenberg, D.L. Pouquet, A. Fluid dynamics Kinetic energy Kinetics Reynolds number Boussinesq equations Isotropic energy Large scale anisotropy Power-law behavior Rotating turbulence Scale separation Spatial resolution Vertical direction Anisotropy solution and solubility anisotropy computer simulation energy transfer Fourier analysis kinetics rotation solution and solubility theoretical model Anisotropy Computer Simulation Energy Transfer Fourier Analysis Kinetics Models, Theoretical Rotation Solutions 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 10243 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. © 2014 American Physical Society. Fil:Mininni, P.D. Universidad de Buenos Aires. Facultad de Ciencias Exactas y Naturales; Argentina. JOUR info:eu-repo/semantics/openAccess http://creativecommons.org/licenses/by/2.5/ar http://hdl.handle.net/20.500.12110/paper_15393755_v90_n2_p_Marino
institution Universidad de Buenos Aires
institution_str I-28
repository_str R-134
collection Biblioteca Digital - Facultad de Ciencias Exactas y Naturales (UBA)
topic Fluid dynamics
Kinetic energy
Kinetics
Reynolds number
Boussinesq equations
Isotropic energy
Large scale anisotropy
Power-law behavior
Rotating turbulence
Scale separation
Spatial resolution
Vertical direction
Anisotropy
solution and solubility
anisotropy
computer simulation
energy transfer
Fourier analysis
kinetics
rotation
solution and solubility
theoretical model
Anisotropy
Computer Simulation
Energy Transfer
Fourier Analysis
Kinetics
Models, Theoretical
Rotation
Solutions
spellingShingle Fluid dynamics
Kinetic energy
Kinetics
Reynolds number
Boussinesq equations
Isotropic energy
Large scale anisotropy
Power-law behavior
Rotating turbulence
Scale separation
Spatial resolution
Vertical direction
Anisotropy
solution and solubility
anisotropy
computer simulation
energy transfer
Fourier analysis
kinetics
rotation
solution and solubility
theoretical model
Anisotropy
Computer Simulation
Energy Transfer
Fourier Analysis
Kinetics
Models, Theoretical
Rotation
Solutions
Marino, R.
Mininni, P.D.
Rosenberg, D.L.
Pouquet, A.
Large-scale anisotropy in stably stratified rotating flows
topic_facet Fluid dynamics
Kinetic energy
Kinetics
Reynolds number
Boussinesq equations
Isotropic energy
Large scale anisotropy
Power-law behavior
Rotating turbulence
Scale separation
Spatial resolution
Vertical direction
Anisotropy
solution and solubility
anisotropy
computer simulation
energy transfer
Fourier analysis
kinetics
rotation
solution and solubility
theoretical model
Anisotropy
Computer Simulation
Energy Transfer
Fourier Analysis
Kinetics
Models, Theoretical
Rotation
Solutions
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 10243 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. © 2014 American Physical Society.
format JOUR
author Marino, R.
Mininni, P.D.
Rosenberg, D.L.
Pouquet, A.
author_facet Marino, R.
Mininni, P.D.
Rosenberg, D.L.
Pouquet, A.
author_sort Marino, R.
title Large-scale anisotropy in stably stratified rotating 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
url http://hdl.handle.net/20.500.12110/paper_15393755_v90_n2_p_Marino
work_keys_str_mv AT marinor largescaleanisotropyinstablystratifiedrotatingflows
AT mininnipd largescaleanisotropyinstablystratifiedrotatingflows
AT rosenbergdl largescaleanisotropyinstablystratifiedrotatingflows
AT pouqueta largescaleanisotropyinstablystratifiedrotatingflows
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