Detection of langmuir solitons: implications for type III burst emission mechanisms at 2ωₚₑ

dc.contributor.authorThejappa, G.
dc.contributor.authorStone, R. G.
dc.contributor.authorGoldstein, Melvyn
dc.date.accessioned2023-11-07T19:14:34Z
dc.date.available2023-11-07T19:14:34Z
dc.date.issued1996-03
dc.description.abstractWe present the experimental verification of existing theoretical models of emission mechanisms of solar type III bursts at the second harmonic of the plasma frequency, ω ₚₑ . This study is based on the detection of Langmuir and envelope solitons by the Ulysses spacecraft inside three type III burst source regions. We show that the oscillating-two-stream instability, coherent radiation by Langmuir solitons and stochastic phase mixing of the Langmuir waves in the strong turbulence regime are the appropriate emission mechanisms at 2ω ₚₑ .en_US
dc.description.urihttps://link.springer.com/article/10.1007/BF00644054en_US
dc.format.extent4 pagesen_US
dc.genrejournal articlesen_US
dc.identifierdoi:10.13016/m2gftx-0qfs
dc.identifier.citationThejappa, G., Stone, R.G. & Goldstein, M.L. Detection of langmuir solitons: implications for type III burst emission mechanisms at 2ωₚₑ . Astrophys Space Sci 243, 195–198 (1996). https://doi.org/10.1007/BF00644054en_US
dc.identifier.urihttps://doi.org/10.1007/BF00644054
dc.identifier.urihttp://hdl.handle.net/11603/30576
dc.language.isoen_USen_US
dc.publisherSpringeren_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.titleDetection of langmuir solitons: implications for type III burst emission mechanisms at 2ωₚₑen_US
dc.typeTexten_US
dcterms.creatorhttps://orcid.org/0000-0002-5317-988Xen_US

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