Formation of Nonlinear Stationary Structures in Ionospheric Plasma

Manna, Gobinda; Dey, S; Goswami, Jyotirmoy; Chandra, Swarniv; Sarkar, Jit; Gupta, Amrita

doi:10.1109/tps.2022.3166685

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Cited by 11 publications

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“…Finally, simulating in main loop with drift (and applied some periodic boundary conditions) we obtain the twostream instability in phase space. Such instabilities can be explained elaborately in the light of studies carried out by some authors [53][54][55][56][57] using dynamical systems.…”

Section: Appendixmentioning

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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