Physics of plasma radiation

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dc.contributor.authorChian, A.
dc.contributor.authorAbalde, J.
dc.contributor.authorAlves, M.
dc.contributor.authorDe Moraes, M.
dc.contributor.authorRempel, E.
dc.contributor.authorRizzato, F.
dc.date.issued2003
dc.description.abstractWe present a theory of the fundamental plasma emission of type-III solar radio bursts. Starting from the generalized Zakharov equations, considering the pump wave as a pair of oppositely propagating Langmuir waves with different amplitudes, and the excitation of electromagnetic and induced Langmuir waves, we obtain a general dispersion relation for the coupled waves. We numerically solve the general dispersion relation using the pump wave amplitude and plasma parameters observed in the interplanetary medium.
dc.description.statementofresponsibilityAbraham C.-L. Chian, José R. Abalde, Maria Virgínia Alves, Márcio A. E. De Moraes, Erico L. Rempel, and Felipe B. Rizzato
dc.identifier.citationProgress of Theoretical Physics Supplement, 2003; 151(151):226-233
dc.identifier.doi10.1143/PTPS.151.226
dc.identifier.issn0375-9687
dc.identifier.orcidChian, A. [0000-0002-8932-0793]
dc.identifier.urihttp://hdl.handle.net/2440/11243
dc.language.isoen
dc.publisherProgress Theoretical Physics Publication Office
dc.rightsCopyright (c) 2003 Progress of Theoretical Physics
dc.source.urihttps://doi.org/10.1143/ptps.151.226
dc.titlePhysics of plasma radiation
dc.typeJournal article
pubs.publication-statusPublished

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