Determination of the properties of magnetic turbulence in radio sources

Astronomy and Astrophysics – Astronomy

Scientific paper

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Interstellar Magnetic Fields, Magnetohydrodynamic Turbulence, Nonuniform Magnetic Fields, Radio Sources (Astronomy), Synchrotron Radiation, Plasma Density, Radio Galaxies, Stochastic Processes, Stokes Law Of Radiation

Scientific paper

The transport of polarized synchrotron radiation in a source possessing a highly irregular magnetic field, as proposed by Laing has been considered. The transport equation has been solved in a special case, relating the observable correlation functions in the Stokes parameters Q and U to the correlation functions of magnetic field and plasma density in the source. A rough application of the results to observations of the radio galaxy 3C 166 indicates that the turbulent scale length may be a few percent of the lobe size.

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