2020
DOI: 10.1007/s11277-020-07831-z
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Optimum Power Allocation Based on Channel Conditions in Optical Satellite Downlinks

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Cited by 6 publications
(9 citation statements)
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“…The optical channel for the downlink follows the LN distribution considering weak scintillation conditions. By incorporating the quantum efficiencies of the transmitter η LEO and receiver η OGS , the atmospheric transmittance T Atm , the gains of transmitter g LEO and receiver g OGS , the large-scale path loss PL, the small-scale loss due to scintillation e 2X s where X s is the log-amplitude of the optical wave and hence Gaussian (normally) distributed, the optical channel is expressed by [4,21]:…”
Section: System Modelmentioning
confidence: 99%
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“…The optical channel for the downlink follows the LN distribution considering weak scintillation conditions. By incorporating the quantum efficiencies of the transmitter η LEO and receiver η OGS , the atmospheric transmittance T Atm , the gains of transmitter g LEO and receiver g OGS , the large-scale path loss PL, the small-scale loss due to scintillation e 2X s where X s is the log-amplitude of the optical wave and hence Gaussian (normally) distributed, the optical channel is expressed by [4,21]:…”
Section: System Modelmentioning
confidence: 99%
“…In particular, the optical noise is a zero mean, a constant variance random variable that describes the environmental optical interference. It incorporates the background radiation from the various celestial bodies, the amplified spontaneous emission (ASE) from optical preamplifiers and the electronic detection noise [4,21]. By using narrow passband optical filters and small field-of-view telescopes the receiver can eliminate the ambient background radiation and ASE, while the thermal and shot noises can be considered as additive white Gaussian noise [2].…”
Section: System Modelmentioning
confidence: 99%
“…For mitigating the cloud occlusion, site diversity can be used [8]. Received irradiance scintillation is created from rapid changes in wind speed, pressure, and temperature, which in turn induce changes in the refractive index [10][11][12]. The impact of scintillation depends primarily upon the time of day, the elevation angle of the link, and the altitude of the station [10][11][12].…”
Section: Introductionmentioning
confidence: 99%
“…Received irradiance scintillation is created from rapid changes in wind speed, pressure, and temperature, which in turn induce changes in the refractive index [10][11][12]. The impact of scintillation depends primarily upon the time of day, the elevation angle of the link, and the altitude of the station [10][11][12]. In the daytime, at low elevation angles and low-altitude stations (denser atmosphere), turbulence is more extreme [10][11][12].…”
Section: Introductionmentioning
confidence: 99%
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