15th European Turbulence Conference 2015
August 25-28th, 2015, Delft, The Netherlands
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Universal Statistical Properties of Inertial-particle Trajectories in Three-dimensional, Homogeneous, Isotropic, Fluid Turbulence


Go-down etc15 Tracking Number 173

Presentation:
Session: Lagrangian aspects of turbulence 1
Room: Room F
Session start: 10:30 Wed 26 Aug 2015

Akshay Bhatnagar   akshayphy@gmail.com
Affifliation: Centre for Condensed Matter Theory, Department of Physics, Indian Institute of Science, Bangalore 560012, India.

Anupam Gupta   anupam1509@gmail.com
Affifliation: University of Rome ``Tor Vergata'', Rome, Italy.

Dhrubaditya Mitra   dhruba.mitra@gmail.com
Affifliation: NORDITA, Roslagstullsbacken 23, SE-10691 Stockholm, Sweden.

Prasad Perlekar   perlekar@tifrh.res.in
Affifliation: TIFR Centre for Interdisciplinary Sciences, 21 Brundavan Colony, Narsingi, Hyderabad 500075, India.

Rahul Pandit   rahul@physics.iisc.ernet.in
Affifliation: Centre for Condensed Matter Theory, Department of Physics, Indian Institute of Science, Bangalore 560012, India.


Topics: - Transport and mixing, - Lagrangian aspects of turbulence

Abstract:

We obtain new universal statistical properties of heavy-particle trajectories in three-dimensional, statistically steady, homogeneous, and isotropic turbulent flows by direct numerical simulations. We show that the probability distribution functions (PDFs) $P(\phi)$, of the angle $\phi$ between the Eulerian velocity ${\bf u}$ and the particle velocity ${\bf v}$, at a point and time, scales as $P(\phi) \sim \phi^{-\gamma}$, with a new universal exponent $\gamma \simeq 4$. The PDFs of the trajectory curvature $\kappa$ and modulus $\theta$ of the torsion $\vartheta$ scale, respectively, as $P(\kappa) \sim \kappa^{-h_\kappa}$, as $\kappa \to \infty$, and $P(\theta) \sim \theta^{-h_\theta}$, as $\theta \to \infty$, with exponents $h_\kappa \simeq 2.5$ and $h_\theta \simeq 3$ that do not depend on the Stokes number $St$. We also show that $\gamma$, $h_\kappa$ and $h_\theta$ can be obtained by using simple stochastic models. We show that the number $N_I(t,St)$ of points (up until time $t$), at which $\vartheta$ changes sign, is such that $n_I(St) \equiv \lim_{t\to\infty} \frac{N_I(t,St)}{t} \sim St^{-\Delta}$, with $\Delta \simeq 0.4$ a universal exponent.