Comment on “Kinetic Simulations of Magnetized Turbulence in Astrophysical Plasmas”

W. H. Matthaeus, S. Servidio, and P. Dmitruk
Phys. Rev. Lett. 101, 149501 – Published 1 October 2008

Abstract

A Comment on the Letter by G. G. Howes et al., Phys. Rev. Lett. 100, 065004 (2008). The authors of the Letter offer a Reply.

  • Figure
  • Received 21 April 2008

DOI:https://doi.org/10.1103/PhysRevLett.101.149501

©2008 American Physical Society

Authors & Affiliations

W. H. Matthaeus1, S. Servidio1, and P. Dmitruk2

  • 1Department of Physics and Astronomy University of Delaware Newark, Delaware 19716, USA
  • 2Departamento de Fisica Facultad de Ciencias Exactas y Naturales Universidad de Buenos Aires Argentina

Comments & Replies

Howes et al. Reply:

G. G. Howes, S. C. Cowley, W. Dorland, G. W. Hammett, E. Quataert, A. A. Schekochihin, and T. Tatsuno
Phys. Rev. Lett. 101, 149502 (2008)

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Original Article

Kinetic Simulations of Magnetized Turbulence in Astrophysical Plasmas

G. G. Howes, W. Dorland, S. C. Cowley, G. W. Hammett, E. Quataert, A. A. Schekochihin, and T. Tatsuno
Phys. Rev. Lett. 100, 065004 (2008)

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Issue

Vol. 101, Iss. 14 — 3 October 2008

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