Polarization of the radio emission of pulsars

Details Polarization of the radio emission of pulsars Polarization of the radio emission of pulsars

Oct 1975

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1975sva....19..171o&link_type=abstract

(Astronomicheskii Zhurnal, vol. 52, Mar.-Apr. 1975, p. 278-281.) Soviet Astronomy, vol. 19, no. 2, 1975, p. 171-173. Translatio

Astronomy and Astrophysics

Astronomy

3

Polarized Electromagnetic Radiation, Pulsars, Radio Emission, Relativistic Plasmas, Stellar Atmospheres, Cosmic Plasma, Magnetospheres, Stellar Magnetic Fields, Stellar Radiation

Scientific paper

It is shown analytically that the strong linear polarization of the radio emission from the pulsar PSR 0833-45 may be due to the influence on radio propagation of an ultrarelativistic magnetically active plasma in its magnetosphere. A model of a pulsar magnetosphere is presented which demonstrates that such a plasma can serve as a polaroid for radio emission in the case of quasi-transverse propagation. The parameters of the plasma in the magnetosphere of PSR 0833-45 are estimated by applying this polarization mechanism.

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