Dissipation in Poynting‐Flux–dominated Flows: The σ‐Problem of the Crab Pulsar Wind
Author:
Publisher
American Astronomical Society
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
http://stacks.iop.org/0004-637X/591/i=1/a=366/pdf
Reference58 articles.
1. Arons, J. 1983 in Electron-Positron Pairs in Astrophysics, ed. M. L. Burns, A. K. Harding, & R. Ramaty (New York: AIP), 163
2. An axisymmetric magnetohydrodynamic model for the Crab pulsar wind bubble
3. On the MHD effects on the force-free monopole outflow
4. Biskamp, D. 2000, Magnetic Reconnection in Plasmas (Cambridge: Cambridge Univ. Press)
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