A mechanism for electrostatic solitary waves observed in the reconnection jet

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dc.contributor.author Lakhina, G.S.
dc.contributor.author Singh, Satyavir
dc.contributor.author Rubia, R.
dc.date.accessioned 2022-09-12T08:45:53Z
dc.date.available 2022-09-12T08:45:53Z
dc.date.issued 2022
dc.identifier.citation 44th COSPAR Scientific Assembly. Held 16-24 July, 2022. Online at https://www.cosparathens2022.org/. Abstract D3.3-0005-22 en_US
dc.identifier.uri http://library.iigm.res.in:8080/xmlui/handle/123456798/341
dc.description.abstract Magnetospheric Multiscale spacecraft (MMS) mission has observed electrostatic solitary waves (ESWs) in the reconnection jet region in the Earth's magnetotail. An ion-acoustic soliton model, based on Sagdeev pseudopotential technique, is proposed to explain these ESWs. The reconnection jet plasma is modeled by a three-component magnetized plasma consisting of hot electrons and two cold ion beams streaming parallel and anti-parallel to the magnetic field, B respectively. The model predicts four types of ion-acoustic solitons, namely, two fast and two slow ion-acoustic solitons, where one of each type propagates parallel and another anti-parallel to the ambient magnetic field, respectively. The model predicts positive potential solitons with amplitudes ∼ (51-539) V, associated bipolar electric fields with amplitudes in the range of ∼ (3-69) mV m −1 , and the soliton widths of ∼  (4.5-10.3) Debye lengths. Theoretical predictions are found to be in good agreement with the observed characteristics of ESWs in the reconnection jet region by MMS mission. en_US
dc.language.iso en en_US
dc.subject Electrostatic solitary waves en_US
dc.subject Magnetotail-Earth en_US
dc.subject Ion acoustic solitons en_US
dc.title A mechanism for electrostatic solitary waves observed in the reconnection jet en_US
dc.type Other en_US


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