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dc.contributor.authorRufai, O.R.
dc.contributor.authorBharuthram, R.
dc.contributor.authorSingh, S.V.
dc.contributor.authorLakhina, G.S.
dc.date.accessioned2017-10-27T05:27:07Z
dc.date.accessioned2021-02-12T09:58:13Z-
dc.date.available2016-10-27T05:27:07Z
dc.date.available2021-02-12T09:58:13Z-
dc.date.issued2016
dc.identifier.citationAdvances in Space Research, 57, p. 813–820, doi: 10.1016/j.asr.2015.11.021en_US
dc.identifier.urihttp://localhost:8080/xmlui/handle/123456789/1003-
dc.description.abstractArbitrary amplitude nonlinear low frequency electrostatic soliton and supersoliton structures are studied in magnetized fourcomponent auroral plasmas composed of a cold singly charged oxygen-ion fluid, Boltzmann distribution of hot protons and two distinct group of electron species. Using the Sagdeev pseudo-potential technique, the characteristics of obliquely propagating nonlinear structures are investigated analytically and numerically. The model supports the evolution of soliton and supersoliton structures in the auroral acceleration region. Depending on the parametric region, the positive and negative potential solitons coexists at lower Mach numbers, but at higher Mach numbers only negative potential solitons and supersolitons can exist. The presence of hot protons restricted the Mach number of the nonlinear structures to exist only at the subsonic region. The present investigation concurs with the Swedish Viking satellite observations in the auroral region.en_US
dc.language.isoenen_US
dc.subjectLow frequency wavesen_US
dc.subjectSolitons and supersolitonsen_US
dc.subjectMagnetized plasmasen_US
dc.subjectMach numbersen_US
dc.subjectAuroral zoneen_US
dc.subjectEarth’s magnetosphereen_US
dc.titleObliquely propagating ion-acoustic solitons and supersolitons in four-component auroral plasmasen_US
dc.typeArticleen_US
dc.identifier.accession091545
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