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A LES-LANGEVIN MODEL. Colls: R. Dolganov and J-P Laval N. Kevlahan E.-J. Kim F. Hersant J. Mc Williams S. Nazarenko P. Sullivan J. Werne. B. Dubrulle Groupe Instabilite et Turbulence CEA Saclay. IS IT SUFFICIENT TO KNOW BASIC EQUATIONS?. Giant convection cell. Dissipation
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A LES-LANGEVIN MODEL Colls: R. Dolganov and J-P Laval N. Kevlahan E.-J. Kim F. Hersant J. Mc Williams S. Nazarenko P. Sullivan J. Werne B. Dubrulle Groupe Instabilite et Turbulence CEA Saclay
IS IT SUFFICIENT TO KNOW BASIC EQUATIONS? Giant convection cell Dissipation scale Solar spot Granule 0.1 km Waste of computational resources Time-scale problem Necessity of small scale parametrization
Influence of decimated scales Typical time at scale l: Decimated scales (small scales) vary very rapidly We may replace them by a noise with short time scale Generalized Langevin equation
Obukhov Model Simplest case No mean flow Large isotropic friction No spatial correlations Gaussian velocities Richardson’s law Kolmogorov’s spectra LES: Langevin
Influence of decimated scales: transport Stochastic computation Turbulent viscosity AKA effect
Refined comparison Additive noise True turbulence Gaussianity Weak intermittency Non-Gaussianité Forte intermittence Iso-vorticity Spectrum PDF of increments LES: Langevin
LOCAL VS NON-LOCAL INTERACTIONS • Navier-Stokes equations : two types of triades NON-LOCAL LOCAL L L l
NON-LOCAL TURBULENCE E U Analogy with MHD equations: small scale grow via « dynamo » effect k Conservation laws In inviscid case
A PRIORI TESTS IN NUMERICAL SIMULATIONS 2D TURBULENCE << Non-local Local small/small scales Local large/ large scales 3D TURBULENCE
DYNAMICAL TESTS IN NUMERICAL SIMULATIONS 2D RDT 2D DNS 3D RDT 3D DNS
THE RDT MODEL Equation for large-scale velocity Linear stochastic inhomogeneous equation (RDT) Reynolds stresses Equation for small scale velocity Forcing (energy cascade) Turbulent viscosity Computed (numerics) or prescribed (analytics)
THE FORCING Iso-vorticity Iso-force PDF of increments Correlations
TURBULENT VISCOSITY SES RDT DNS
k x LANGEVIN EQUATION AND LAGRANGIAN SCHEME Décomposition into wave packets The wave packet moves with the fluid Its wave number is changed by shear Its amplitude depends on forces coupling (cascade) “multiplicative noise” friction “additive noise”
COMPARISON DNS/SES Fast numerical 2D simulation Shear flow Computational time 10 days 2 hours phi_m obs DNS Lagrangian model (Laval, Dubrulle, Nazarenko, 2000) Hersant, Dubrulle, 2002
SES SIMULATIONS SES Experiment Hersant, 2003 DNS
LANGEVIN MODEL: derivation Equation for small scale velocity Turbulent viscosity Forcing Isoforce PDF LES: Langevin
Equation for Reynolds stress with Forcing due To cascade Advection Distorsion By non-local interactions Generalized Langevin equation LES: Langevin
Performances Comparaison DNS: 384*384*384 et LES: 21*21*21 Intermittency Spectrum LES: Langevin
Performances (2) s probability Q vs R LES: Langevin
THE MODEL IN SHEARED GEOMETRY Basic equations RDT equations for fluctuations with stochastic forcing Equation for mean profile
ANALYTICAL PREDICTIONS Mean flow dominates Fluctuations dominates Low Re
TORQUE IN TAYLOR-COUETTE No adjustable parameter Dubrulle and Hersant, 2002