Depolarization of emission of some pulsars

Details Depolarization of emission of some pulsars Depolarization of emission of some pulsars

Jun 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985a%26a...147..184g&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 147, no. 1, June 1985, p. 184, 185.

Astronomy and Astrophysics

Astrophysics

3

Depolarization, Emission Spectra, Linear Polarization, Magnetic Field Configurations, Pulsars, Stellar Magnetic Fields, Circular Polarization, Line Of Sight, Stellar Rotation

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 the radiation reaching an observer at any one time may represent contributions from several particle bunches moving relativistically along different magnetic field lines and radiating incoherently. These assumptions are used to explain the minimum of linear polarization appearing near the profile centre of some pulsars.

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