Electrostatic solitary structures in presence of non-thermal electrons and a warm electron beam on the auroral field lines

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dc.contributor.author Singh, S.V.
dc.contributor.author Lakhina, G.S.
dc.contributor.author Bharuthram, R.
dc.contributor.author Pillay, S.R.
dc.date.accessioned 2016-03-30T10:11:08Z
dc.date.accessioned 2021-02-12T09:53:46Z
dc.date.available 2016-03-30T10:11:08Z
dc.date.available 2021-02-12T09:53:46Z
dc.date.issued 2011
dc.identifier.citation Physics of Plasmas, v.18,122306, 2011, doi: 10.1063/1.3671955 en_US
dc.identifier.uri http://localhost:8080/xmlui/handle/123456789/866
dc.description.abstract Electrostatic 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.iso en en_US
dc.subject Electrostatic solitary waves en_US
dc.subject Non-thermal electrons en_US
dc.subject Plasma waves en_US
dc.subject Potential solitary en_US
dc.subject Auroral field en_US
dc.subject Earth’s Magnetosphere en_US
dc.title Electrostatic solitary structures in presence of non-thermal electrons and a warm electron beam on the auroral field lines en_US
dc.type Article en_US
dc.identifier.accession 091188


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