paper

Lagrangian acceleration in fully developed turbulence and its Eulerian decompositions

arXiv:2210.15877 · doi:10.1103/PhysRevFluids.8.L032601

Abstract

We study the properties of various Eulerian contributions to fluid particle acceleration by using well-resolved direct numerical simulations of isotropic turbulence, with the grid resolution as high as and the Taylor-scale Reynolds number in the range between 140 and 1300. The variance of convective acceleration, when normalized by Kolmogorov scales, increases linearly with , consistent with simple theoretical arguments, but very strongly differing from phenomenological predictions of Kolmogorov's hypothesis as well as Eulerian multifractal models. The scaling of the local acceleration is also linear to the leading order, but more complex in detail. The strong cancellation between the local and convective acceleration -- faithful to the random sweeping hypothesis -- results in the variance of the Lagrangian acceleration increasing only as , as recently shown by Buaria \& Sreenivasan [Phys. Rev. Lett. 128, 234502 (2022)]. The acceleration variance is dominated by irrotational pressure gradient contributions, whose variance also follows an scaling; the solenoidal viscous contributions are relatively small and follow a , consistent with Eulerian multifractal predictions.

8 pages, 3 figures

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