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dc.contributor.authorBharuthram, R.
dc.contributor.authorReddy, R.V.
dc.contributor.authorLakhina, G.S.
dc.contributor.authorSingh, N.
dc.date.accessioned2015-09-21T11:16:23Z
dc.date.accessioned2021-02-12T09:28:37Z
dc.date.available2015-09-21T11:16:23Z
dc.date.available2021-02-12T09:28:37Z
dc.date.issued2002
dc.identifier.citationPhysica Scripta, v.T98, p.137-140, 2002, doi: 10.1238/Physica.Topical.098a00137en_US
dc.identifier.urihttp://localhost:8080/xmlui/handle/123456789/452
dc.description.abstractThe nonlinear evolution of low frequency electrostatic waves in a magnetised plasma is investigated for parameters characteristic of the auroral acceleration region. Our model consists of Boltzmann electrons and warm ions. Using fluid theory, a nonlinear evolution equation is derived for the wave potential. Numerical solutions show the existence of sinusoidal, sawtooth or bipolar waveforms. The effects of plasma parameters on the wave amplitude are examined, in particular the effect of a finite ion temperature.en_US
dc.language.isoenen_US
dc.subjectNonlinear wavesen_US
dc.subjectAuroral plasmasen_US
dc.subjectElectrostatic wavesen_US
dc.titleLow frequency nonlinear waves in the auroral plasmaen_US
dc.typeArticleen_US
dcterms.sourcedoi: 10.1238/Physica.Topical.098a00137
dc.identifier.accession090958
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