102 research outputs found

    Turbulence and turbulent pattern formation in a minimal model for active fluids

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    Active matter systems display a fascinating range of dynamical states, including stationary patterns and turbulent phases. While the former can be tackled with methods from the field of pattern formation, the spatio-temporal disorder of the active turbulence phase calls for a statistical description. Borrowing techniques from turbulence theory, we here establish a quantitative description of correlation functions and spectra of a minimal continuum model for active turbulence. Further exploring the parameter space, we also report on a surprising type of turbulence-driven pattern formation far beyond linear onset: the emergence of a dynamic hexagonal vortex lattice state after an extended turbulent transient, which can only be explained taking into account turbulent energy transfer across scales.Comment: Supplemental videos available at https://youtu.be/gbf6cRho03w https://youtu.be/n0qUUhAUJFQ https://youtu.be/LGmamkM012

    Extreme Lagrangian acceleration in confined turbulent flow

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    A Lagrangian study of two-dimensional turbulence for two different geometries, a periodic and a confined circular geometry, is presented to investigate the influence of solid boundaries on the Lagrangian dynamics. It is found that the Lagrangian acceleration is even more intermittent in the confined domain than in the periodic domain. The flatness of the Lagrangian acceleration as a function of the radius shows that the influence of the wall on the Lagrangian dynamics becomes negligible in the center of the domain and it also reveals that the wall is responsible for the increased intermittency. The transition in the Lagrangian statistics between this region, not directly influenced by the walls, and a critical radius which defines a Lagrangian boundary layer, is shown to be very sharp with a sudden increase of the acceleration flatness from about 5 to about 20

    Zonal flow generation and its feedback on turbulence production in drift wave turbulence

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    Plasma turbulence described by the Hasegawa-Wakatani equations has been simulated numerically for different models and values of the adiabaticity parameter C. It is found that for low values of C turbulence remains isotropic, zonal flows are not generated and there is no suppression of the meridional drift waves and of the particle transport. For high values of C, turbulence evolves toward highly anisotropic states with a dominant contribution of the zonal sector to the kinetic energy. This anisotropic flow leads to a decrease of a turbulence production in the meridional sector and limits the particle transport across the mean isopycnal surfaces. This behavior allows to consider the Hasegawa-Wakatani equations a minimal PDE model which contains the drift-wave/zonal-flow feedback loop prototypical of the LH transition in plasma devices.Comment: 14 pages, 7 figure

    Reynolds number effect on the velocity increment skewness in isotropic turbulence

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    Second and third order longitudinal structure functions and wavenumber spectra of isotropic turbulence are computed using the EDQNM model and compared to results of the multifractal formalism. At the highest Reynolds number available in windtunnel experiments, Rλ=2500R_\lambda=2500, both the multifractal model and EDQNM give power-law corrections to the inertial range scaling of the velocity increment skewness. For EDQNM, this correction is a finite Reynolds number effect, whereas for the multifractal formalism it is an intermittency correction that persists at any high Reynolds number. Furthermore, the two approaches yield realistic behavior of second and third order statistics of the velocity fluctuations in the dissipative and near-dissipative ranges. Similarities and differences are highlighted, in particular the Reynolds number dependence

    Dynamics of spectrally truncated inviscid turbulence

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    The evolution of the turbulent energy spectrum for the inviscid spectrally truncated Euler equations is studied by closure calculations. The observed behavior is similar to the one found in direct numerical simulations [Cichowlas, Bona\"ititi, Debbasch, and Brachet, Phys. Rev. Lett. 95, 264502 (2005)]. A Kolmogorov spectral range and an equipartition range are observed simultaneously. Between these two ranges a "quasi-dissipative" zone is present in the kinetic energy spectrum. The time evolution of the wave number that marks the beginning of the equipartition range is analyzed and it is shown that spectral nonlocal interactions are governing this evolution

    The role of coherent vorticity in turbulent transport in resistive drift-wave turbulence

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    The coherent vortex extraction method, a wavelet technique for extracting coherent vortices out of turbulent flows, is applied to simulations of resistive drift-wave turbulence in magnetized plasma (Hasegawa-Wakatani system). The aim is to retain only the essential degrees of freedom, responsible for the transport. It is shown that the radial density flux is carried by these coherent modes. In the quasi-hydrodynamic regime, coherent vortices exhibit depletion of the polarization-drift nonlinearity and vorticity strongly dominates strain, in contrast to the quasiadiabatic regime

    Space-local Navier--Stokes turbulence

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    We investigate the physical-space locality of interactions in three-dimensional incompressible turbulent flow. To that, we modify the nonlinear terms of the vorticity equation such that the vorticity field is advected and stretched by the locally induced velocity. This space-local velocity field is defined by the truncated Biot--Savart law, where only the neighboring vorticity field in a sphere of radius RR is integrated. We conduct direct numerical simulations of the space-local system to investigate its statistics in the inertial range. We observe a standard E(k)k5/3E(k) \propto k^{-5/3} scaling of the energy spectrum associated with an energy cascade for scales smaller than the space-local domain size kR1k \gg R^{-1}. This result is consistent with the assumption Kolmogorov's 1941 paper made for the space-locality of the nonlinear interactions. The enstrophy production is suppressed for larger scales kR1k \ll R^{-1}, and for these scales, the system exhibits a scaling consistent with a conservative enstrophy cascade.Comment: 22 pages, 8 figure

    Minimal modeling of the intrinsic cycle of turbulence driven by steady forcing

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    Quasi-Cyclic Behavior (QCB) is a common feature of various laminar and turbulent flows. We conduct Direct Numerical Simulations (DNS) of three-dimensional flow driven by the steady Taylor--Green forcing to find a silent similarity between a stable periodic flow at a small Reynolds number (Re\mathrm{Re}) and turbulent QCB at higher Re\mathrm{Re}. These two temporal dynamics are continuously connected by varying Re\mathrm{Re}. A close examination of the periodic flow allows the formulation of a simple three-equation model, representing the evolution of Fourier modes in three distinct scales. The model reproduces the continuously connected periodic solution and QCB when Re\mathrm{Re} is varied. We find that non-local triad interactions are necessary to maintain the periodic solution and QCB. Bifurcation analyses illustrate that the model can also reproduce several critical features of turbulence, such as sudden relaminarization of transient chaos. These findings suggest that the model is not specific to the studied flow in a periodic domain but is of more general importance in investigating turbulence in different flow configurations

    Rapid generation of angular momentum in bounded magnetized plasma

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    Direct numerical simulations of two-dimensional decaying MHD turbulence in bounded domains show the rapid generation of angular momentum in nonaxisymmetric geometries. It is found that magnetic fluctuations enhance this mechanism. On a larger time scale, the generation of a magnetic angular momentum, or angular field, is observed. For axisymmetric geometries, the generation of angular momentum is absent; nevertheless, a weak magnetic field can be observed. The derived evolution equations for both the angular momentum and angular field yield possible explanations for the observed behavior
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