Kinetic Alfvén Wave Turbulence and Transport through a Reconnection Diffusion Region

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Citation of Original Publication

Chaston, C. C., J. R. Johnson, M. Wilber, M. Acuna, M. L. Goldstein, and H. Reme. “Kinetic Alfvén Wave Turbulence and Transport through a Reconnection Diffusion Region.” Physical Review Letters 102, no. 1 (January 8, 2009): 015001. https://doi.org/10.1103/PhysRevLett.102.015001.

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This work was written as part of one of the author's official duties as an Employee of the United States Government and is therefore a work of the United States Government. In accordance with 17 U.S.C. 105, no copyright protection is available for such works under U.S. Law.
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Abstract

We demonstrate from observations that kinetic Alfvén waves may play an important role in facilitating magnetic reconnection. These waves radiate outwards from the diffusion region oblique to the magnetic field in a conelike pattern delimited by the X line separatrices with outward energy fluxes equivalent to that contained in the outstreaming ions. It is shown that the wave vectors reverse across the X and symmetry lines and have a large out of plane component. We estimate that these waves drive significant transport through the diffusion region.