Polarization of pulsar radio emission

Details Polarization of pulsar radio emission Polarization of pulsar radio emission

Apr 1975

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1975azh....52..278o&link_type=abstract

Astronomicheskii Zhurnal, vol. 52, Mar.-Apr. 1975, p. 278-281. In Russian.

Astronomy and Astrophysics

Astronomy

2

Polarized Electromagnetic Radiation, Pulsars, Radio Emission, Relativistic Plasmas, Stellar Atmospheres, Cosmic Plasma, Pulsar 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.

Affiliated with

Also associated with

No associations

Rating

Polarization of pulsar radio emission does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Polarization of pulsar radio emission, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Polarization of pulsar radio emission will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-947740