How are orthogonally polarized modes generated?

Details How are orthogonally polarized modes generated? How are orthogonally polarized modes generated?

Feb 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008aipc..983...47m&link_type=abstract

40 YEARS OF PULSARS: Millisecond Pulsars, Magnetars and More. AIP Conference Proceedings, Volume 983, pp. 47-50 (2008).

Physics

Radiation Mechanisms, Polarization, Pulsars, Neutron Stars, Magnetohydrodynamics And Plasmas

Scientific paper

The observation of elliptically polarized OPMs as a characteristic feature of single radio pulses poses a major challenge to conventional pulsar theory, which implies emission in a single linearly polarized mode. It is argued that elliptically polarized OPMs can result as a propagation effect in an oscillatory model for the pulsar magnetosphere, in which the electrons and positrons have a periodic counter streaming motion in which their maximum Lorentz factor is γ~106.

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