Calculation of the pulse profiles in the case of curvature radiation

Details Calculation of the pulse profiles in the case of curvature radiation Calculation of the pulse profiles in the case of curvature radiation

Oct 1980

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980afz....16..750m&link_type=abstract

(Astrofizika, vol. 16, Oct.-Dec. 1980, p. 750-756.) Astrophysics, vol. 16, no. 4, Apr. 1981, p. 430-433. Translation.

Astronomy and Astrophysics

Astrophysics

1

Electromagnetic Wave Transmission, Plasma Radiation, Pulsar Magnetospheres, Pulsars, Pulsed Radiation, Stellar Magnetic Fields, Magnetic Field Configurations, Optical Thickness, Plasma-Electromagnetic Interaction, Polar Caps, Relativistic Electron Beams, Stellar Models, Stellar Spectrophotometry, Waveforms

Scientific paper

Pulse profiles are calculated for different frequencies on the basis of the polar cap model under the assumption that radiation of the given frequency is generated at a fixed level in the pulsar magnetosphere. For two pulsars (PSR 0525 and PSR 1133), comparison of the calculated and observed profiles leads to an estimate of the energy of the emitting electrons and the position of the line of sight relative to the axis of the radiation cone.

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