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Phys. Rev. Lett. 101, 149501 (2008) [1 pages]

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

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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

Received 21 April 2008; published 1 October 2008

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.

© 2008 The American Physical Society

URL:
http://link.aps.org/doi/10.1103/PhysRevLett.101.149501
DOI:
10.1103/PhysRevLett.101.149501
PACS:
52.35.Ra, 52.65.Tt, 96.50.Tf

See Also

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

Original Article: G. G. Howes, W. Dorland, S. C. Cowley, G. W. Hammett, E. Quataert, A. A. Schekochihin, and T. Tatsuno, Kinetic Simulations of Magnetized Turbulence in Astrophysical Plasmas, Phys. Rev. Lett. 100, 065004 (2008).