Theory of polarized radiation scattering in a randomly inhomogeneous magnetoplasma

Details Theory of polarized radiation scattering in a randomly inhomogeneous magnetoplasma Theory of polarized radiation scattering in a randomly inhomogeneous magnetoplasma

Jan 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992sval...18...37k&link_type=abstract

Soviet Astronomy Letters, Vol. 18, p. 37; Pis'ma v Astronomicheskii Zhurnal (ISSN 0320-0108), vol. 18, no. 1, Jan. 1992, p. 87-9

Astronomy and Astrophysics

Astronomy

Circular Polarization, Cosmic Rays, Electromagnetic Scattering, Polarized Electromagnetic Radiation, Radio Emission, Brightness Distribution, Nonuniform Plasmas, Plasma Frequencies, Stokes Law Of Radiation

Scientific paper

Theoretical analysis of the spatial coherence of the polarized emission from cosmic radio sources shows that in a randomly inhomogeneous magnetoplasma a slight circular polarization of the initially nonpolarized emission arises when the observation points are separated. The presence of the magnetic field fluctuations results in opposite phase velocity shifts of clockwise and counterclockwise waves, which in turn causes a relative linear polarization growth when the interferometer baseline increases.

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