Energy dissipation in turbulent reconnection

Author:

Bandyopadhyay R.1ORCID,Chasapis A.2ORCID,Matthaeus W. H.34ORCID,Parashar T. N.5ORCID,Haggerty C. C.6ORCID,Shay M. A.34ORCID,Gershman D. J.7ORCID,Giles B. L.7ORCID,Burch J. L.8ORCID

Affiliation:

1. Department of Astrophysical Sciences, Princeton University, Princeton, New Jersey 08544, USA

2. Laboratory for Atmospheric and Space Physics, University of Colorado Boulder, Boulder, Colorado 80309, USA

3. Department of Physics and Astronomy, University of Delaware, Newark, Delaware 19716, USA

4. Bartol Research Institute, University of Delaware, Newark, Delaware 19716, USA

5. School of Chemical and Physical Sciences, Victoria University of Wellington, Wellington 6012, New Zealand

6. Institute for Astronomy, University of Hawaii, Honolulu, Hawaii 96822, USA

7. NASA Goddard Space Flight Center, Greenbelt, Maryland 20771, USA

8. Southwest Research Institute, San Antonio, Texas 78238, USA

Funder

National Aeronautics and Space Administration

NASA

Publisher

AIP Publishing

Subject

Condensed Matter Physics

Reference66 articles.

1. D. Montgomery et al., Report of the NASA Plasma Turbulence Explorer Study Group ( NASA, Jet Propulsion Laboratory, Pasadena, CA, 1980), Vol. 715–778.

2. The Solar Wind as a Turbulence Laboratory

3. Who Needs Turbulence?

4. The multi-scale nature of the solar wind

5. Study of energy conversion and partitioning in the magnetic reconnection layer of a laboratory plasmaa)

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