Orthogonal polarization in pulsar radio emission

Details Orthogonal polarization in pulsar radio emission Orthogonal polarization in pulsar radio emission

Oct 1975

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1975pasau...2..334m&link_type=abstract

(Astronomical Society of Australia, Annual General Meeting, 9th, Parkes, New South Wales, Australia, May 14-16, 1975.) Astronomi

Astronomy and Astrophysics

Astronomy

7

Polarized Electromagnetic Radiation, Pulsars, Radio Emission, Stellar Radiation, Orthogonality, Polarization Characteristics, Radiant Flux Density, Stellar Magnetic Fields, Synchrotron Radiation

Scientific paper

Characteristics of orthogonal polarization in integrated profiles for two pulsars are discussed and aspects of orthogonal polarization in individual pulses are investigated. Mechanisms for which emission at two orthogonal angles is a natural feature are considered, taking into account the self-absorption effect seen in synchrotron sources and a radiation mechanism which can operate in two modes, one polarized parallel to the field and one perpendicular.

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