The Sigma Problem of the Crab Pulsar Wind

@inproceedings{Kirk2003TheSP,
  title={The Sigma Problem of the Crab Pulsar Wind},
  author={J. Kirk and O. Skjaeraasen},
  year={2003}
}
Flows in which energy is transported predominantly as Poynting flux are thought to occur in pulsars, gamma-ray bursts, and relativistic jets from compact objects. The fluctuating component of the magnetic field in such a flow can in principle be dissipated by magnetic reconnection and used to accelerate the flow. We investigate how rapidly this transition can take place by implementing into a global MHD model that uses a thermodynamic description of the plasma, explicit, physically motivated… Expand

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