Physics – Fluid Dynamics
Scientific paper
2009-02-03
Phys. Rev. E 80, 046306 (2009)
Physics
Fluid Dynamics
14 pages, 20 figures. This version of the article has been accepted for publication in PRE. Note though that the PRE paper for
Scientific paper
10.1103/PhysRevE.80.046306
On the basis of various DNS of turbulent channel flows the following picture is proposed. (i) At a height y from the y = 0 wall, the Taylor microscale \lambda is proportional to the average distance l_s between stagnation points of the fluctuating velocity field, i.e. \lambda(y) = B_1 l_s(y) with B_1 constant, for \delta_\nu << y \lesssim \delta. (ii) The number density n_s of stagnation points varies with height according to n_s = C_s y_+^{-1} / \delta_\nu^3 where C_s is constant in the range \delta_\nu << y \lesssim \delta. (iii) In that same range, the kinetic energy dissipation rate per unit mass, \epsilon = 2/3 E_+ u_\tau^3 / (\kappa_s y) where E_+ is the total kinetic energy per unit mass normalised by u_\tau^2 and \kappa_s = B_1^2 / C_s is the stagnation point von K\'arm\'an coefficient. (iv) In the limit of exceedingly large Re_\tau, large enough for the production to balance dissipation locally and for -
Dallas Vassilios
Hewitt Geoffrey F.
Vassilicos John Christos
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