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Rapid polarization variability in intense sources

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dc.contributor.author Gangadhara, R. T
dc.contributor.author Krishan, V
dc.date.accessioned 2008-07-09T09:23:59Z
dc.date.available 2008-07-09T09:23:59Z
dc.date.issued 1995-02
dc.identifier.citation Astrophysical Journal, Part 1, Vol. 440, No. 1, p. 116 – 127 en
dc.identifier.issn 0004-637X
dc.identifier.uri http://hdl.handle.net/2248/2610
dc.description.abstract We have recently reported the polarization changes of the intense electromagnetic radiation, in active galactic nuclei and pulsars, due to stimulated Raman scattering. In this paper, we show that the incident and the Raman-scattered radiation, when superimposed, exhibit highly complex and variable polarization patterns, some of which could account for the observed polarization variability in intense sources. Further, if the ratio of the frequencies of the incident and the scattered radiation is an irrational number, the electric field of the superimposed radiation traces a quasi-periodic rotation. The modulation of the Raman-scattered sideband modes, with even small perturbations due to the thermal radiation or the Raman cascade, would lead to chaotic rotation of the electric field of the superimposed radiation. en
dc.format.extent 1800753 bytes
dc.format.mimetype application/pdf
dc.language.iso en en
dc.publisher The American Astronomical Society en
dc.relation.uri http://adsabs.harvard.edu/abs/1995ApJ...440..116G en
dc.subject Active Galactic Nuclei en
dc.subject Astronomical Models en
dc.subject Electromagnetic Radiation en
dc.subject Plasma-Electromagnetic Interaction en
dc.subject Polarization (Waves) en
dc.subject Pulsars en
dc.subject Raman Spectra en
dc.subject Space Plasmas en
dc.subject Variability en
dc.subject Electric Fields en
dc.subject Electromagnetic Wave Transmissionn en
dc.subject Electron Plasman en
dc.subject Mathematical Models en
dc.subject Plasma Density en
dc.subject Plasma Waves en
dc.title Rapid polarization variability in intense sources en
dc.type Article en


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