Lagrangian statistics are reported from a direct numerical simulation database with grid resolution up to 20483 and Taylor-scale Reynolds number approximately 650. The approach to Lagrangian Kolmogorov similarity at high Reynolds number is studied using both the velocity structure function and frequency spectrum. A significant scaling range is observed for the latter which is consistent with recent estimates of 6 - 7 for the scaling constant C-0. In contrast to some previous results at low Reynolds number, the current results suggest that at high Reynolds number the dissipation autocorrelation is a two-scale process influenced by both the Lagrangian velocity integral time scale and Kolmogorov time scale. Results on the logarithm of the pseudo-dissipation are in support of its modeling as a diffusion process with one-time Gaussian statistics. As the Reynolds number increases, the statistics of dissipation and enstrophy become more similar while their logarithms have significantly longer time scales.
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Univ Glasgow, James Watt Sch Engn, Glasgow G12 8QQ, Lanark, ScotlandLawrence Livermore Natl Lab, 4 Ivy Lane,7000 East Ave, Livermore, CA 94550 USA
Busse, A.
Mueller, W-C
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TU Berlin, Ctr Astron & Astrophys, ER 3-2,Hardenbergstr 36, D-10623 Berlin, GermanyLawrence Livermore Natl Lab, 4 Ivy Lane,7000 East Ave, Livermore, CA 94550 USA
机构:
Univ Roma Tor Vergata, Dept Phys, I-00133 Rome, Italy
Univ Roma Tor Vergata, Ist Nazl Fis Nucl, I-00133 Rome, ItalyUniv Roma Tor Vergata, Dept Phys, I-00133 Rome, Italy
Benzi, R.
Biferale, L.
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Univ Roma Tor Vergata, Dept Phys, I-00133 Rome, Italy
Univ Roma Tor Vergata, Ist Nazl Fis Nucl, I-00133 Rome, ItalyUniv Roma Tor Vergata, Dept Phys, I-00133 Rome, Italy
Biferale, L.
Fisher, R.
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Univ Massachusetts, Dept Phys, Dartmouth, MA 02740 USAUniv Roma Tor Vergata, Dept Phys, I-00133 Rome, Italy
Fisher, R.
Lamb, D. Q.
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Univ Chicago, Ctr Astrophys Thermonucl Flashes, Chicago, IL 60637 USA
Univ Chicago, Dept Astron & Astrophys, Chicago, IL 60637 USAUniv Roma Tor Vergata, Dept Phys, I-00133 Rome, Italy