Plasma Shock Wave in Gamma-Ray Bursts: Nonlinear Phenomena and Radiative Process

Ballav, Swastik; Das, Ansuman; Pramanick, Suman; Chandra, Swarniv

doi:10.1109/tps.2021.3112178

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Cited by 24 publications

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“…Our study lies in that velocity regime on which two-stream instability leads to a strong acceleration of planetary ions which are very energetic in the range of suprathermal energies [27]. Some newer simulation studies based on homotopy [28][29][30][31][32] could provide some additional information.…”

Section: Initial Conditionsmentioning

confidence: 99%

Two-stream plasma instability as a potential mechanism for particle escape from the Venusian ionosphere

et al. 2022

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In this work we investigate the possibility of two-stream instability in the Venusian atmosphere to lead to momentum transfer to subsequent escape of Hydrogen and Oxygen ions from the ionosphere. We employ the hydrodynamic model and obtain the linear dispersion relation from which the two-stream instability is studied. Further the interaction of solar wind with the ions of Venus ionosphere from which the instability sets in, has been studied with the data from ASPERA-4 of Venus Express (VEX). The data supports the fact that the two-stream instability can provide sufficient energy to accelerate ions to escape velocity of the planet.

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