Non-linear high-frequency waves in the magnetosphere

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dc.contributor.authorMoolla, S.en_US
dc.contributor.authorBharuthram, R.en_US
dc.contributor.authorSingh, S.V.en_US
dc.contributor.authorLakhina, G. S.en_US
dc.date.accessioned2026-07-24T06:35:51Z
dc.date.issued2003
dc.description.abstractUsing fluid theory, a set of equations is derived for non-linear high-frequency waves propagating oblique to an external magnetic field in a three-component plasma consisting of hot electrons, cold electrons and cold ions. For parameters typical of the Earth’s magnetosphere, numerical solutions of the governing equations yield sinusoidal, sawtooth or bipolar wave-forms for the electric field.en_US
dc.identifier.citationPramana-Journal of Physics, v.61/6, p.1209-1214, 2003, doi: 10.1007/BF02704418en_US
dc.identifier.other90767
dc.identifier.urihttps://repository.iigm.res.in/handle/123456789/2256
dc.languageenen_US
dc.subjectMagnetosphereen_US
dc.subjectBipolaren_US
dc.subjectSawtooth wave-formsen_US
dc.subjectElectric fieldsen_US
dc.subjectNon-linear high-frequency wavesen_US
dc.titleNon-linear high-frequency waves in the magnetosphereen_US
dc.typeArticleen_US

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