Parametric generation of the magnetic field and activity in the Crab Nebula

Details Parametric generation of the magnetic field and activity in the Crab Nebula Parametric generation of the magnetic field and activity in the Crab Nebula

Apr 1982

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982sogru.106...49l&link_type=abstract

Akademiia Nauk Gruzinskoi SSR, Soobshcheniia, vol. 106, Apr. 1982, p. 49-52. In Russian.

Physics

Brightness Distribution, Crab Nebula, Interstellar Magnetic Fields, Plasma-Electromagnetic Interaction, Pulsars, Synchrotron Radiation, Electron Plasma, Magnetic Dipoles, Maxwell Equation, Plasma Resonance, Relativistic Particles

Scientific paper

A new mechanism for the formation of wisps in the Crab Nebula is proposed. It is shown that, where resonance conditions are satisfied in the nebula plasma, an intense electromagnetic wave can generate a stationary magnetic field. The excited magnetic field leads to an increase in local synchrotron radiation, which can be associated with the appearance of wisps.

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