Evolution of rogue waves in dusty plasmas
- Department of Mathematics, Faculty of Science, Damietta University, New Damietta 34517 (Egypt)
- Department of Physics, Faculty of Science, Port Said University, Port Said 42521 (Egypt)
- (BUE), El-Shorouk City, Cairo (Egypt)
- Department of Physics, Faculty of Science, Damietta University, New Damietta 34517 (Egypt)
The evolution of rogue waves associated with the dynamics of positively charged dust grains that interact with streaming electrons and ions is investigated. Using a perturbation method, the basic set of fluid equations is reduced to a nonlinear Schrödinger equation (NLSE). The rational solution of the NLSE is presented, which proposed as an effective tool for studying the rogue waves in Jupiter. It is found that the existence region of rogue waves depends on the dust-acoustic speed and the streaming densities of the ions and electrons. Furthermore, the supersonic rogue waves are much taller than the subsonic rogue waves by ∼25 times.
- OSTI ID:
- 22408385
- Journal Information:
- Physics of Plasmas, Vol. 22, Issue 4; Other Information: (c) 2015 AIP Publishing LLC; Country of input: International Atomic Energy Agency (IAEA); ISSN 1070-664X
- Country of Publication:
- United States
- Language:
- English
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