A geometrical depolarization of pulsar radiation

Details A geometrical depolarization of pulsar radiation A geometrical depolarization of pulsar radiation

Feb 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985ap%26ss.109..381g&link_type=abstract

Astrophysics and Space Science (ISSN 0004-640X), vol. 109, no. 2, Feb. 1985, p. 381-386.

Statistics

Computation

Depolarization, Polarized Electromagnetic Radiation, Pulsars, Stellar Radiation, Computational Astrophysics, Linear Polarization, Polar Caps

Scientific paper

It is assumed that pulsar radiation originates in a polar cap region and that the emission mechanism is curvature radiation. It is further assumed that radiation reaching an observer at any time may represent contributions from several particle bunches moving relativistically along different magnetic field lines and radiating mutually incoherently. These assumptions are used to explain the minimum of linear polarization appearing near the profile centre of some pulsars.

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