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 – Published 1 October 2008

Abstract

A Reply to the Comment by W. H. Matthaeus, S. Servidio, and P. Dmitruk.

  • Received 6 June 2008

DOI:https://doi.org/10.1103/PhysRevLett.101.149502

©2008 American Physical Society

Authors & Affiliations

G. G. Howes1, S. C. Cowley2, W. Dorland3, G. W. Hammett4, E. Quataert5, A. A. Schekochihin6, and T. Tatsuno3

  • 1University of Iowa, USA
  • 2Culham Science Centre, United Kingdom
  • 3University of Maryland, USA
  • 4Princeton Plasma Physics Laboratory, USA
  • 5University of California, USA
  • 6Imperial College, United Kingdom

Comments & Replies

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

W. H. Matthaeus, S. Servidio, and P. Dmitruk
Phys. Rev. Lett. 101, 149501 (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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Vol. 101, Iss. 14 — 3 October 2008

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