Fully nonlinear dust-ion-acoustic excitation in Jupiter ionosphere
El-qumaish, Q., Tolba, R., Moslem, W., El-Labany, S. (2023). Fully nonlinear dust-ion-acoustic excitation in Jupiter ionosphere. EKB Journal Management System, 4(3), 495-505. doi: 10.21608/ajbas.2023.179308.1136
Qumaish El-qumaish; Reda Tolba; Waleed Moslem Moslem; Salah El-Labany. "Fully nonlinear dust-ion-acoustic excitation in Jupiter ionosphere". EKB Journal Management System, 4, 3, 2023, 495-505. doi: 10.21608/ajbas.2023.179308.1136
El-qumaish, Q., Tolba, R., Moslem, W., El-Labany, S. (2023). 'Fully nonlinear dust-ion-acoustic excitation in Jupiter ionosphere', EKB Journal Management System, 4(3), pp. 495-505. doi: 10.21608/ajbas.2023.179308.1136
El-qumaish, Q., Tolba, R., Moslem, W., El-Labany, S. Fully nonlinear dust-ion-acoustic excitation in Jupiter ionosphere. EKB Journal Management System, 2023; 4(3): 495-505. doi: 10.21608/ajbas.2023.179308.1136

Fully nonlinear dust-ion-acoustic excitation in Jupiter ionosphere

Alfarama Journal of Basic & Applied Sciences
Article 10, Volume 4, Issue 3, July 2023, Page 495-505  XML PDF (785.17 K)
Document Type: Original Article
DOI: 10.21608/ajbas.2023.179308.1136
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Authors
Qumaish El-qumaish1; Reda Tolba2; Waleed Moslem Moslem email orcid 3; Salah El-Labany4
1Department of Physics, Faculty of Science, Amran University- Yemen
2Centre for Theoretical Physics, The British University in Egypt (BUE), El-Shorouk city, Cairo, Egypt
3Department of Physics, Faculty of Science, Port Said University, Port Said, Egypt
4Department of Physics, Faculty of Science, Damietta University, New Damietta, Egypt
Abstract
Fully nonlinear solitary wave structure of dust-ion-acoustic waves are investigated in
a five-component plasma consisting of positive proton beam from solar wind, positive ion
fluid, two electrons population, one of them from the solar wind and stationary positive
dust grains. The physical parameters in the system such as, proton beam-to-positive
ion temperature and density ratios, as well as solar wind electron number density play
an important role in the profile of the large amplitude dust-ion-acoustic solitary waves.
Using pseudo-potential approach (Sagdeev potential) the basic equations are reduced to
one evolution equation called an energy equation. The latter has been analysed and solved
numerically to obtain an arbitrary amplitude solitary profile as well as the possible regions
for the existence waves. The solution of energy equation presents a positive potential,
which corresponds to a compressive wave profile. The findings of this investigation are
used to interpret the electrostatic arbitrary solitary waves that may be observed in the
Jupiter ionosphere.
Keywords
dust-ion-acoustic waves; Jupiter ionosphere; large amplitude solitary waves
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