A systematic bias in the calculation of spectral density from a 3D spatial grid
Computational Physics
2015-06-23 v1
Abstract
The energy spectral density , where is the spatial wave number, is a well-known diagnostic of homogeneous turbulence and magnetohydrodynamic turbulence. However in most of the curves plotted by different authors, some systematic kinks can be observed at , and . We claim that these kinks have no physical meaning, and are in fact the signature of the method which is used to estimate from a 3D spatial grid. In this paper we give another method, in order to get rid of the spurious kinks and to estimate much more accurately.
Keywords
Cite
@article{arxiv.1410.8263,
title = {A systematic bias in the calculation of spectral density from a 3D spatial grid},
author = {Rodion Stepanov and Franck Plunian and Mouloud Kessar and Guillaume Balarac},
journal= {arXiv preprint arXiv:1410.8263},
year = {2015}
}
Comments
4 pages, in PRE