Angular distribution of gamma-ray radiation from magnetic polar caps of fast pulsars.

Details Angular distribution of gamma-ray radiation from magnetic polar caps of fast pulsars. Angular distribution of gamma-ray radiation from magnetic polar caps of fast pulsars.

Aug 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991icrc....2..432s&link_type=abstract

22. International Cosmic Ray Conference (ICRC-22), Vol. 2, p. 432 - 435

Physics

Pulsars: Gamma Rays, Pulsars: Radiation Mechanisms

Scientific paper

A numerical investigation on the angular distribution of the gamma-ray radiation emitted by relativistic primary particles flying from the magnetic polar caps of a fast pulsar with an inclination of χ ≠ 0 between its rotating axis and magnetic axis is presented on the basis of the classical theory of radiation. It is indicated that the major factors which intensely influence the orientation characteristics of the gamma-ray radiation are the curvature of the magnetic line and the energy dissipation of the primary particles. The considerable distortion of the magnetic line will lead to a certain amount of the directivity dispersion of the radiation.

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