On the mechanism of the formation of the polarization characteristics of pulsar radiation

Details On the mechanism of the formation of the polarization characteristics of pulsar radiation On the mechanism of the formation of the polarization characteristics of pulsar radiation

Jan 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989plap.work..277k&link_type=abstract

In ESA, Proceedings of an International School and Workshop on Plasma Astrophysics, Volume 1 p 277-280 (SEE N89-24910 18-75)

Astronomy and Astrophysics

Astrophysics

Polarization Characteristics, Pulsars, Stellar Radiation, Astronomical Models, Magnetohydrodynamic Stability, Mathematical Models, Stellar Magnetic Fields

Scientific paper

A model of radiation is used to explain characteristics of individual
pulses of pulsars. Mode changing, existence of two orthogonal
polarization modes, and rapid change of position angles from pulse to
pulse are treated.

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