Show simple item record

dc.contributor.authorAli, M.
dc.contributor.authorOrgura, K.
dc.contributor.authorMinami, K.
dc.contributor.authorDestler, William
dc.contributor.authorGranatstein, V.
dc.date.accessioned2009-07-15T15:33:48Z
dc.date.available2009-07-15T15:33:48Z
dc.date.issued1992-04
dc.identifier.citationPhysics of Fluids, vol. 4, no. 4, April, 1992en_US
dc.identifier.urihttp://hdl.handle.net/1850/10165
dc.description.abstractAbsolute instability in a plasma-filled backward wave oscillator with sinusoidally corrugated slow wave structure driven by an intense relativistic electron beam has been analyzed numerically. The maximum spatial growth rate of the plasma-filled waveguide is found to be larger than that of an optimally designed vacuum structure. The excitation of a finite length structure is investigated. Although the spatial growth rates obtained in the linear theory increase with plasma density in the finite length plasma-filled structure for the fundamental TM01 mode of oscillation, negative global spatial growth rates prevent the coherent oscillation for intermediate ranges of plasma density, beam current, and even for structure length.en_US
dc.language.isoen_USen_US
dc.publisherAmerican Institute of Physicsen_US
dc.relation.ispartofseriesvol. 4en_US
dc.relation.ispartofseriesno. 4en_US
dc.titleLinear analysis of a finite length plasma-filled backward wave oscillatoren_US
dc.typeArticleen_US


Files in this item

Thumbnail
Thumbnail
Thumbnail
Thumbnail

This item appears in the following Collection(s)

Show simple item record