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Frequency Spectra Fluctuations in the Radio Interferometry of Polarized Radiation

Published online by Cambridge University Press:  26 May 2016

M.R. Olyak
M.R. Olyak*
Affiliation:
Institute of Radio Astronomy of Ukrainian National Academy of Sciences, 4 Krasnoznamennaya, Kharkov, Ukraine

Abstract

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The presence of a longitudinal magnetic field is shown to lead to the appearance of an additional component of the frequency spectrum of the linearly polarized emission. This component is proportional to the spectrum of normal waves phase difference fluctuations. The fluctuations spectra baseline dependence of a linear polarized radiation is periodical near zero frequency, one is absent in the high frequency ranges and such dependence has different character in magnetoactive plasma with electron density irregularities and in plasma with a random magnetic field.

Type
Part 7: Pulsars and other Compact Galactic Objects
Information
Symposium - International Astronomical Union , Volume 199: The Universe at Low Radio Frequencies , 2002 , pp. 402 - 403
Copyright
Copyright © Astronomical Society of the Pacific 2002 

References

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