Some implications of the polar-cap model of pulsar magnetospheres

Details Some implications of the polar-cap model of pulsar magnetospheres Some implications of the polar-cap model of pulsar magnetospheres

Aug 1979

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1979pazh....5..393i&link_type=abstract

(Pis'ma v Astronomicheskii Zhurnal, vol. 5, Aug. 1979, p. 393-397.) Soviet Astronomy Letters, vol. 5, July-Aug. 1979, p. 211-213

Astronomy and Astrophysics

Astronomy

2

Atmospheric Models, Pulsar Magnetospheres, Pulsars, Stellar Atmospheres, Electron Energy, Magnetospheric Electron Density, Polar Caps, Stellar Magnetic Fields

Scientific paper

The relation between mean pulse width and period predicted by the polar-cap model is consistent with the results of the 408-MHz pulsar survey. When this model is applied to data measured at other frequencies, the level at which radiation is generated in the pulsar magnetosphere is found to rise toward lower frequencies. The energy and density of the electrons in the emission regions are estimated.

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