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dc.contributor.authorSingh, S.V.
dc.contributor.authorDevanandhan, S.
dc.contributor.authorLakhina, G.S.
dc.contributor.authorBharuthram, R.
dc.date.accessioned2015-10-28T09:09:45Z
dc.date.accessioned2021-02-12T09:39:36Z-
dc.date.available2015-10-28T09:09:45Z
dc.date.available2021-02-12T09:39:36Z-
dc.date.issued2013
dc.identifier.citationPhys. Plasmas, v.20, 012306, 2013; doi: 10.1063/1.4776710en_US
dc.identifier.urihttp://localhost:8080/xmlui/handle/123456789/670-
dc.description.abstractObliquely propagating ion-acoustic soliatry waves are examined in a magnetized plasma composed of kappa distributed electrons and fluid ions with finite temperature. The Sagdeev potential approach is used to study the properties of finite amplitude solitary waves. Using a quasi-neutrality condition, it is possible to reduce the set of equations to a single equation (energy integral equation), which describes the evolution of ion-acoustic solitary waves in magnetized plasmas. The temperature of warm ions affects the speed, amplitude, width, and pulse duration of solitons. Both the critical and the upper Mach numbers are increased by an increase in the ion temperature. The ion-acoustic soliton amplitude increases with the increase in superthermality of electrons. For auroral plasma parameters, the model predicts the soliton speed, amplitude, width, and pulse duration, respectively, to be in the range of (28.7–31.8) km/s, (0.18–20.1) mV/m; (590–167) m, and (20.5–5.25) ms, which are in good agreement with Viking observations.en_US
dc.language.isoenen_US
dc.subjectIon temperatureen_US
dc.subjectSolitary wavesen_US
dc.subjectSuperthermal electronsen_US
dc.subjectPlasma wavesen_US
dc.subjectIon-acoustic soliatry wavesen_US
dc.titleEffect of ion temperature on ion-acoustic solitary waves in a magnetized plasma in presence of superthermal electronsen_US
dc.typeArticleen_US
dc.identifier.accession091329
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