Polarization mode coupling in radio pulsars

Details Polarization mode coupling in radio pulsars Polarization mode coupling in radio pulsars

Jul 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983aipc..101..199s&link_type=abstract

IN: Positron-election pairs in astrophysics; Proceedings of the Workshop, Greenbelt, MD, January 6-8, 1983 (A85-31276 13-90). Ne

Astronomy and Astrophysics

Astrophysics

Circular Polarization, Coupled Modes, Polarized Electromagnetic Radiation, Pulsars, Boundary Layer Plasmas, Cosmic Plasma, Elliptical Polarization, Polar Caps, Stellar Magnetic Fields

Scientific paper

Mode coupling (polarization limiting) has been proposed as an explanation for the orthogonally polarized radiation (OPR) observed from pulsars. Using a simplified magnetospheric model it is shown that it cannot account for the presence of circular polarization in the OPR phenomenon. Mode coupling occurs much closer to the star than the point at which the normal modes of the plasma become significantly elliptically polarized.

Affiliated with

Also associated with

No associations

Rating

Polarization mode coupling in radio pulsars 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 mode coupling in radio pulsars, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Polarization mode coupling in radio pulsars will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1626641