On the theory of the type III burst exciter

dc.contributor.authorSmith, Robert A.
dc.contributor.authorGoldstein, Melvyn
dc.contributor.authorPapadopoulos, Konstantinos
dc.date.accessioned2023-11-02T17:58:37Z
dc.date.available2023-11-02T17:58:37Z
dc.date.issued1976-02
dc.description.abstractIn situ satellite observations of type III burst exciters at 1 AU show that the beam does not evolve into a plateau in velocity space, contrary to the prediction quasilinear theory. The observations can be explained by a theory that includes mode coupling effects due to excitation of the parametric oscillating two-stream instability and its saturation by anomalous resistivity. The time evolution of the beam velocity distribution is included in the analysis.en_US
dc.description.urihttps://link.springer.com/article/10.1007/BF00149880en_US
dc.format.extent13 pagesen_US
dc.genrejournal articlesen_US
dc.identifierdoi:10.13016/m2ibq7-wts2
dc.identifier.citationSmith, Robert A., Melvyn L. Goldstein, and Konstantinos Papadopoulos. “On the Theory of the Type III Burst Exciter.” Solar Physics 46, no. 2 (February 1, 1976): 515–27. https://doi.org/10.1007/BF00149880.en_US
dc.identifier.urihttps://doi.org/10.1007/BF00149880
dc.identifier.urihttp://hdl.handle.net/11603/30502
dc.language.isoen_USen_US
dc.publisherSpringer Natureen_US
dc.relation.isAvailableAtThe University of Maryland, Baltimore County (UMBC)
dc.relation.ispartofUMBC Goddard Planetary Heliophysics Institute (GPHI)
dc.rightsThis work was written as part of one of the author's official duties as an Employee of the United States Government and is therefore a work of the United States Government. In accordance with 17 U.S.C. 105, no copyright protection is available for such works under U.S. Law.en_US
dc.rightsPublic Domain Mark 1.0*
dc.rights.urihttp://creativecommons.org/publicdomain/mark/1.0/*
dc.titleOn the theory of the type III burst exciteren_US
dc.typeTexten_US
dcterms.creatorhttps://orcid.org/0000-0002-5317-988Xen_US

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