Probability density of irradiance for electromagnetic waves propagating through turbulent magnetized plasma (002).pdf (319.26 kB)
Probability density of irradiance for electromagnetic waves propagating through turbulent magnetized plasma
journal contribution
posted on 2023-06-10, 04:20 authored by Yousef M Shishter, Rupert YoungRupert Young, Falah AliFalah AliNumerous physical mediums can be modelled as turbulent magnetized plasma, for example, the solar corona, and the ionosphere. Scintillation effects on the intensity of electromagnetic beam wave propagating through magnetized plasma necessitate the introduction of a statistical distribution valid over a large range of scintillation conditions, and incorporating the plasma physical properties. Under some simplifying assumptions, such a theoretical model can be derived based on the Rytov solution, the external magnetic field variation, and the space permeating plasma electron density variation. The resultant wave intensity distribution is compared with the Lognormal, Rician, and the Nakagami distributions for different scintillations conditions. The work presented in this paper is applicable to the analysis and design of optical wireless communication links through the ionosphere and deep space plasma.
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- Published
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- Accepted version
Journal
International Journal of Communication SystemsISSN
1074-5351Publisher
WileyExternal DOI
Article number
e5294Department affiliated with
- Engineering and Design Publications
Full text available
- No
Peer reviewed?
- Yes
Legacy Posted Date
2022-07-26First Compliant Deposit (FCD) Date
2022-07-28Usage metrics
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