Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/2758
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dc.contributor.authorGangadhara, R. T-
dc.contributor.authorKrishan, V-
dc.contributor.authorShukla, P. K-
dc.date.accessioned2008-07-21T09:22:47Z-
dc.date.available2008-07-21T09:22:47Z-
dc.date.issued1993-05-01-
dc.identifier.citationMonthly Notices of the Royal Astronomical Society, Vol. 262, No. 1, pp. 151 - 163en
dc.identifier.issn0035-8711-
dc.identifier.urihttp://hdl.handle.net/2248/2758-
dc.description.abstractThe modulational instability of a large-amplitude, linearly polarized electromagnetic wave propagating in an electron-positron plasma is considered, including the combined effect of relativistic mass variation of the plasma particles, harmonic generation, and the nonresonant, finite-frequency electrostatic density perturbations, all caused by the large-amplitude radiation field. The radiation from many strong sources, such as AGN and pulsars, has been observed to vary over a host of time-scales. It is possible that the extremely rapid variations in the nonthermal continuum of AGN, as well as in the nonthermal radio radiation from pulsars, can be accounted for by the modulational instabilities to which radiation may be subjected during its propagation out of the emission region.en
dc.format.extent1599306 bytes-
dc.format.mimetypeapplication/pdf-
dc.language.isoenen
dc.publisherRoyal Astronomical Societyen
dc.relation.urihttp://adsabs.harvard.edu/abs/1993MNRAS.262..151Gen
dc.subjectActive galactic nucleien
dc.subjectElectron-positron plasmasen
dc.subjectMagnetohydrodynamic stabilityen
dc.subjectPlasma radiationen
dc.subjectPlasma-electromagnetic interactionen
dc.subjectRelativistic plasmasen
dc.subjectNonuniform plasmasen
dc.subjectPulsarsen
dc.subjectRadio sources (astronomy)en
dc.titleThe modulation of radiation in an electron-positron plasmaen
dc.typeArticleen
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