Electromagnetic instabilities of a relativistic neutral beam with inhomogeneous velocity profile in pulsar magnetospheres

Details Electromagnetic instabilities of a relativistic neutral beam with inhomogeneous velocity profile in pulsar magnetospheres Electromagnetic instabilities of a relativistic neutral beam with inhomogeneous velocity profile in pulsar magnetospheres

Mar 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984afz....20..289k&link_type=abstract

(Astrofizika, vol. 20, Mar.-Apr. 1984, p. 289-294) Astrophysics (ISSN 0571-7132), vol. 20, no. 2, Sept. 1984, p. 153-156. Transl

Astronomy and Astrophysics

Astrophysics

1

Electromagnetic Radiation, Magnetohydrodynamic Stability, Pulsar Magnetospheres, Pulsars, Relativistic Plasmas, Stellar Magnetic Fields, Neutral Beams, Nonuniform Plasmas, Relativistic Velocity, Velocity Distribution

Scientific paper

The Alfven-type instability of electromagnetic waves in pulsar
magnetospheres is investigated. The instability is due to the presence
of a transverse velocity gradient of a beam that flows from an
astronomical object with relativistic velocity.

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