Obliquely propagating ion-acoustic solitons and supersolitons in four-component auroral plasmas

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dc.contributor.author Rufai, O.R.
dc.contributor.author Bharuthram, R.
dc.contributor.author Singh, S.V.
dc.contributor.author Lakhina, G.S.
dc.date.accessioned 2017-10-27T05:27:07Z
dc.date.accessioned 2021-02-12T09:58:13Z
dc.date.available 2016-10-27T05:27:07Z
dc.date.available 2021-02-12T09:58:13Z
dc.date.issued 2016
dc.identifier.citation Advances in Space Research, 57, p. 813–820, doi: 10.1016/j.asr.2015.11.021 en_US
dc.identifier.uri http://localhost:8080/xmlui/handle/123456789/1003
dc.description.abstract Arbitrary 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.iso en en_US
dc.subject Low frequency waves en_US
dc.subject Solitons and supersolitons en_US
dc.subject Magnetized plasmas en_US
dc.subject Mach numbers en_US
dc.subject Auroral zone en_US
dc.subject Earth’s magnetosphere en_US
dc.title Obliquely propagating ion-acoustic solitons and supersolitons in four-component auroral plasmas en_US
dc.type Article en_US
dc.identifier.accession 091545


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