M ay 2 00 5 Transverse velocities , intermittency and asymmetry in fully developed turbulence
نویسنده
چکیده
Self-similar properties of turbulence, suggested by Kolmogorov [2], have been intensively studied for a long time. The theory predicted simple scaling for the longitudinal velocity increments ur = u(x+r)−u(x), namely, 〈|ur| 〉 ∼ r. It became clear, however, that there are corrections to these scalings, usually attributed to intermittency. The only exception is the so-called 4/5thKolmogorov law [3] which is exact in inertial range. According to the law, the third moment, that is the structure function, 〈u3r〉 = Buuu(r) = −4/5εr in inertial range, and this scaling has no intermittency corrections [4]. Nevertheless, more detailed study of this third order structure function proved to be useful in understanding the intermittency. It is indeed important to understand what contribution into the third moment give the tails. It is natural to assume that the main events from the core of P (ur), the PDF, mainly contribute. This is certainly the case for even order structure functions, or for moments like 〈|ur| 〉. As to the odd order moments, we note that 〈u3r〉 6 = 0, while 〈ur〉 = 0. This means that the PDF is asymmetric. However, the core of the PDF may be more or less symmetric, in which case the contribution of the tails would be substantial. And indeed, this asymmetry, described by a ramp-model, also suggest intermittency (in addition to the asymmetry) [1], [5]. Further studies showed that indeed the tails of P (ur), responsible for the intermittency, give a substantial contribution to Buuu [6]. Another way to check this connection between asymmetry and intermittency is to compare directly the PDF for positive and negative parts of ur, and we can see that the asymmetry of the PDF stretches far into the tails [6]. The transverse velocities give additional information about both asymmetry and intermittency, and this paper is devoted to their study. The transverse (vertical) component of the velocity increments vr = v(x+ r)− v(x) is also supposed to possess asymmetry, although 〈v r 〉 = 0. Assuming isotropic turbulence, the only non-vanishing correlation is (see [7], [4])
منابع مشابه
1 5 O ct 2 00 4 Singularity Spectrum of Fully - Developed Turbulence : Parabolic - Profile Model
The parabolic-profile model for the singularity spectrum f(α) of fully-developed turbulence (FDT) is pursued further. This model is shown to provide not only considerable insight into the qualitative aspects of the intermittency problem but also the universal aspects associated with it. The parabolic-profile model also affords, unlike the multi-fractal model, an analytical calculation of probab...
متن کاملar X iv : a st ro - p h / 02 05 28 3 v 1 1 7 M ay 2 00 2 Dust Motions Driven by MHD Turbulence
We discuss the relative grain motions due to MHD turbulence in interstel-lar medium. It has been known for decades that turbulent drag is an efficient way to induce grain relative motions. However, earlier treatments disregarded magnetic field and used Kolmogorov turbulence. Unlike hydro turbulence, MHD turbulence is anisotropic on small scales. Moreover, compressible modes are important for MH...
متن کاملRelative dispersion in fully developed turbulence: the Richardson's law and intermittency corrections.
Relative dispersion in fully developed turbulence is investigated by means of direct numerical simulations. Lagrangian statistics is found to be compatible with Richardson description although small systematic deviations are found. The value of the Richardson constant is estimated as C2 approximately equal to 0.55, in a close agreement with recent experimental findings [S. Ott and J. Mann, J. F...
متن کاملov 2 00 2 On the interaction between velocity increment and energy dissipation in the turbulent cascade
We adress the problem of interactions between the longitudinal velocity increment and the energy dissipation rate in fully developed turbulence. The coupling between these two quantities is experimentally investigated by the theory of stochastic Markovian processes. The so–called Markov analysis allows for a precise characterization of the joint statistical properties of velocity increment and ...
متن کامل2 00 2 On the interaction between velocity increment and energy dissipation in the turbulent cascade
We adress the problem of interactions between the longitudinal velocity increment and the energy dissipation rate in fully developed turbulence. The coupling between these two quantities is experimentally investigated by the theory of stochastic Markovian processes. The so–called Markov analysis allows for a precise characterization of the joint statistical properties of velocity increment and ...
متن کامل