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APS » Journals » Phys. Rev. Lett. » Volume 101 » Issue 14
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Phys. Rev. Lett. 101, 149502 (2008) [1 pages]

Howes et al. Reply:

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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

Received 6 June 2008; published 1 October 2008

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

© 2008 The American Physical Society

URL:
http://link.aps.org/doi/10.1103/PhysRevLett.101.149502
DOI:
10.1103/PhysRevLett.101.149502
PACS:
52.35.Ra, 52.65.Tt, 96.50.Tf

See Also

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).

Original Article: W. H. Matthaeus, S. Servidio, and P. Dmitruk, Comment on “Kinetic Simulations of Magnetized Turbulence in Astrophysical Plasmas”, Phys. Rev. Lett. 101, 149501 (2008).

 
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