Astronomy and Astrophysics – Astrophysics
Scientific paper
Aug 1986
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986esasp.251..429c&link_type=abstract
In ESA Proceedings of the Joint Varenna-Abastumani International School and Workshop on Plasma Astrophysics p 429-433 (SEE N87-
Astronomy and Astrophysics
Astrophysics
Crab Nebula, Magnetohydrodynamic Stability, Magnetostatic Fields, Pulsars, Electron Plasma, Plasma Frequencies, Plasma Pumping, Plasma Resonance
Scientific paper
Generation of quasistatic magnetic fields in electron plasma in the field of strong electromagnetic wave radiation is considered. A sufficiently large pump wave amplitude is required for the creation of electron relativistic motion. When the condition of parametric resonance is fulfilled, i.e., the pump wave frequency is close to plasma frequency, growth rates of instabilities are calculated, and the maximum value of the generated magnetic field is estimated. The mechanism of the appearance of wisps in the Crab Nebula, and observed features of wisps are explained.
Chedia O. V.
Lominadze Jumber G.
Tsikarishvili Elgouja G.
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