Plasma waves propagating along a magnetic field in a strongly anisotropic relativistic plasma

Details Plasma waves propagating along a magnetic field in a strongly anisotropic relativistic plasma Plasma waves propagating along a magnetic field in a strongly anisotropic relativistic plasma

Apr 1979

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1979afz....15..253o&link_type=abstract

(Astrofizika, vol. 15, Apr.-June 1979, p. 253-267.) Astrophysics, vol. 15, no. 2, Oct. 1979, p. 169-178. Translation.

Astronomy and Astrophysics

Astrophysics

Anisotropic Media, Plasma Diffusion, Plasma Waves, Pulsars, Relativistic Plasmas, Stellar Magnetic Fields, Frequency Ranges, Maxwell-Boltzmann Density Function, Velocity Distribution, Wave Propagation

Scientific paper

The paper presents a study made of the dispersion properties of plasma waves propagating along a strong magnetic field in a relativistic plasma with one-dimensional distribution function of the particles. It is shown that undamped plasma waves exist in the frequency range of omegap to omegal. In addition it is demonstrated that weakly damped plasma waves with a phase velocity less than c and a frequency equal to omegal(1 - Delta), with Delta between 0 and 1, exist in a plasma with one-dimensional ultrarelativistic Maxwellian or power distribution function.

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