English

High-Wavenumber Finite Differences and Turbulence Simulations

Astrophysics 2007-05-23 v1

Abstract

We introduce a fluid dynamics algorithm that performs with nearly spectral accuracy, but uses finite-differences instead of FFTs to compute gradients and thus executes 10 times faster. The finite differencing is not based on a high-order polynomial fit. The polynomial scheme has supurb accuracy for low-wavenumber gradients but fails at high wavenumbers. We instead use a scheme tuned to enhance high-wavenumber accuracy at the expense of low wavenumbers, although the loss of low-wavenumber accuracy is negligibly slight. A tuned gradient is capable of capturing all wavenumbers up to 80 percent of the Nyquist limit with an error of no worse than 1 percent. The fact that gradients are based on finite differences enables diverse geometries to be considered and eliminates the parallel communications bottleneck.

Keywords

Cite

@article{arxiv.astro-ph/0402606,
  title  = {High-Wavenumber Finite Differences and Turbulence Simulations},
  author = {Jason Maron},
  journal= {arXiv preprint arXiv:astro-ph/0402606},
  year   = {2007}
}

Comments

20 pages, 7 figures

R2 v1 2026-07-22T08:35:20.519Z