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Reply to Comment on "Spectra of strong magnetohydrodynamic turbulence from high-resolution simulations"

Solar and Stellar Astrophysics 2014-10-07 v1

Abstract

In a Comment by Perez et al (2014) it is claimed that recently published simulations of Beresnyak (2014) are grossly underresolved, compared to theirs, and that Beresnyak (2014) failed to estimate numerical error. Both claims are contrary to the fact. Firstly, as far as numerical resolution is concerned, Beresnyak (2014) was using kmaxη41k_{\rm max}\eta_{41}=1.06 resolution criterion, while Perez et al has been using kmaxη41k_{\rm max}\eta_{41}=0.8. Obviously, 1.06>0.81.06>0.8. Secondly, Beresnyak (2014) have estimated numerical error and found it to be below 3×1033\times 10^{-3}, which is properly explained in the paper. On close inspection of the Comment I have not found a single numerical value or parameter pertaining to the criticized paper, Beresnyak (2014), and it is completely unclear how the Authors came to their conclusions.

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Cite

@article{arxiv.1410.0957,
  title  = {Reply to Comment on "Spectra of strong magnetohydrodynamic turbulence from high-resolution simulations"},
  author = {Andrey Beresnyak},
  journal= {arXiv preprint arXiv:1410.0957},
  year   = {2014}
}

Comments

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