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Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/3840
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dc.contributor.authorKrishan, V-
dc.contributor.authorSivaram, C-
dc.date.accessioned2008-09-23T14:28:43Z-
dc.date.available2008-09-23T14:28:43Z-
dc.date.issued1983-04-
dc.identifier.citationSolar Physics, Vol. 84, No. 1 - 2, pp. 125 - 130en
dc.identifier.issn0038-0938-
dc.identifier.urihttp://hdl.handle.net/2248/3840-
dc.descriptionOpen Access-
dc.description.abstractThe equations describing the linear-acceleration mechanism of radiation emission are generalized and applied to type III and IIIb solar radio bursts. A general expression for the power emitted by an electron in a spatially and temporally periodic electromagnetic/electrostatic field parallel to the ambient magnetic field is derived, allowing for harmonic generation and relaxing the dipole approximation used in previous quantifications of the mechanism. The general expression is used to calculate the radiation due to the electric field generated by saturation-phase beam-plasma instability in the proposed linear-acceleration model of III/IIIb-type solar radio bursts.en
dc.language.isoenen
dc.publisherSpringeren
dc.relation.urihttp://www.springerlink.com/content/vgw72x7538883r6v/en
dc.relation.urihttp://adsabs.harvard.edu/abs/1983SoPh...84..125Ken
dc.subjectElectron Beamsen
dc.subjectHarmonic Generationsen
dc.subjectMagnetohydrodynamic Stabilityen
dc.subjectParticle Accelerationen
dc.subjectSolar Magnetic Fielden
dc.subjectType 3 Burstsen
dc.subjectBeam Interactionsen
dc.subjectEmission Spectraen
dc.subjectParticle Trajectoriesen
dc.subjectPlasma Interactionsen
dc.titleRadio emission by parallel acceleration mechanismen
dc.typeArticleen
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