A new aspect of the hollow-cone model of pulsar emission

Details A new aspect of the hollow-cone model of pulsar emission A new aspect of the hollow-cone model of pulsar emission

Feb 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984a%26a...131...67g&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 131, no. 1, Feb. 1984, p. 67-71.

Astronomy and Astrophysics

Astrophysics

6

Pulsars, Stellar Magnetic Fields, Stellar Models, Stellar Radiation, Computerized Simulation, Polar Caps

Scientific paper

The hollow-cone model of pulsar emission proposed by Komesaroff (1970) is generalized along the lines proposed by Gil (1981, 1982), attributing double-humped mean profiles to tubes of preferred field lines and eliminating the need for a nonradiating hollow zone near the magnetic axis. A numerical simulation is developed to test the mechanisms of emission in this model, and the results are presented in tables and illustrated with simulated pulses and mean profiles.

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