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Faraday rotation measure variations in the Cygnus region and the spectrum of interstellar plasma turbulence
Journal article   Peer reviewed

Faraday rotation measure variations in the Cygnus region and the spectrum of interstellar plasma turbulence

T. Joseph Lazio, Steven R Spangler and James M Cordes
The Astrophysical journal, Vol.363(2), pp.515-527
11/1990
DOI: 10.1086/169362

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Abstract

Linear polarization observations were made of eight double-lobed radio galaxies viewed through the galactic plane in the Cygnus region. These observations have been used to determine intra- and intersource rotation measure differences; in some cases, we have extracted unambiguous rotation measures. The rotation measures are dominated by foreground magnetoionic material. The differences in rotation measure between pairs of sources correlate with angular separation for separations from 10″ to 1°.5. These rotation measure fluctuations are consistent with a model in which the electron density varies on ≈ 0.1-200 pc scales. The amplitudes of these variations are, in turn, consistent with those electron density variations that cause diffractive interstellar scattering on scales less than 1011 cm.

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