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Please use this identifier to cite or link to this item: http://eprint.iitd.ac.in/handle/2074/1948

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dc.contributor.authorJarwal, R K-
dc.contributor.authorSharma, A K-
dc.contributor.authorTripathi, V K-
dc.date.accessioned2006-07-03T05:44:38Z-
dc.date.available2006-07-03T05:44:38Z-
dc.date.issued1999-
dc.identifier.citationPlasma Science, IEEE Transactions on, 27(3), 664 - 667p.en
dc.identifier.urihttp://eprint.iitd.ac.in/dspace/handle/2074/1948-
dc.description.abstractA high power millimeter (mm) wave, in the presence of a magnetic wiggler, produces a large longitudinal ponderomotive force that can accelerate electrons. When a plasma of density n~ncr, where n cr is critical density, is introduced in the interaction region, the ponderomotive force resonantly drives a plasma wave that accelerates electrons to higher energies. However, propagation of the mm wave requires a guide magnetic field; O-mode requiring less field than the X-mode. The plasma wave in this situation goes over to the upper hybrid (UH) mode. A parabolic plasma density profile with minimum on axis provides guiding for the mm wave as well as the UH wave, the latter being more strongly localized than the former. The UH wave, for typical parameters, can accelerate electrons to several tens of megaelectronvoltsen
dc.format.extent92233 bytes-
dc.format.mimetypeapplication/pdf-
dc.language.isoenen
dc.subjectlongitudinal ponderomotive forceen
dc.subjectupper hybrid modeen
dc.subjectmegaelectronvoltsen
dc.titleFeasibility of a plasma-filled inverse free electron laser acceleratoren
dc.typeArticleen
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