Howes et al. Reply
G. G. Howes, S. C. Cowley, W. Dorland, G.W. Hammett, E. Quataert, A., A. Schekochihin, and T. Tatsuno
TL;DR
This paper is a reply to a comment on their previous work about kinetic simulations of magnetized turbulence in astrophysical plasmas, clarifying and defending their original findings.
Contribution
It provides a detailed response to critiques, reaffirming the validity of their kinetic simulation methods and results in astrophysical plasma turbulence.
Findings
Reaffirms the accuracy of their simulation approach
Addresses and clarifies points raised in the comment
Supports the original conclusions on plasma turbulence
Abstract
Howes et al. Reply to Comment on "Kinetic Simulations of Magnetized Turbulence in Astrophysical Plasmas" arXiv:0711.4355
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