Please use this identifier to cite or link to this item: http://library.iigm.res.in:8080/xmlui/handle/123456789/866
Full metadata record
DC FieldValueLanguage
dc.contributor.authorSingh, S.V.
dc.contributor.authorLakhina, G.S.
dc.contributor.authorBharuthram, R.
dc.contributor.authorPillay, S.R.
dc.date.accessioned2016-03-30T10:11:08Z
dc.date.accessioned2021-02-12T09:53:46Z-
dc.date.available2016-03-30T10:11:08Z
dc.date.available2021-02-12T09:53:46Z-
dc.date.issued2011
dc.identifier.citationPhysics of Plasmas, v.18,122306, 2011, doi: 10.1063/1.3671955en_US
dc.identifier.urihttp://localhost:8080/xmlui/handle/123456789/866-
dc.description.abstractElectrostatic solitary waves (ESWs) have been observed by satellites in the auroral region of the Earth’s magnetosphere. These ESWs are found to be having both positive and negative electrostatic potentials. Using the Sagdeeev psuedo-potential technique, arbitrary amplitude electron-acoustic solitary waves/double layers are studied in an unmagnetized plasma consisting of non-thermally distributed hot electrons, fluid cold electrons, a warm electron beam, and ions. The inertia of the warm electrons, and not the beam speed, is essential for the existence of positive potential solitary structures. Existence domains for positive as well as negative potential electrostatic solitons/double layers are obtained. For the typical auroral region parameters, the electric field amplitude of the negative potential solitons is found to be in the range ∼(3–30) mV/m and ∼(5–80) mV/m for the positive potential solitons. For the negative potential solitons/double layers, the amplitudes are higher when their widths are smaller. On the other hand, the amplitude of the positive potential structures increase with their widths.en_US
dc.language.isoenen_US
dc.subjectElectrostatic solitary wavesen_US
dc.subjectNon-thermal electronsen_US
dc.subjectPlasma wavesen_US
dc.subjectPotential solitaryen_US
dc.subjectAuroral fielden_US
dc.subjectEarth’s Magnetosphereen_US
dc.titleElectrostatic solitary structures in presence of non-thermal electrons and a warm electron beam on the auroral field linesen_US
dc.typeArticleen_US
dc.identifier.accession091188
Appears in Collections:UAS_Reprints

Files in This Item:
File Description SizeFormat 
SinghSV_LakhinaGS_PhysicsPlasma_2011.pdfReprint497.44 kBAdobe PDFView/Open


Items in DSpace are protected by copyright, with all rights reserved, unless otherwise indicated.