A mechanism for electrostatic solitary waves observed in the reconnection jet
| 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.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.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:4000/handle/123456798/341 | |
| 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 |