Laser Communication and Propagation Through the Atmosphere and Oceans X 2021
DOI: 10.1117/12.2595727
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Wavefront sensing for terrestrial, underwater, and space-borne free-space optical communications

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Cited by 5 publications
(5 citation statements)
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“…Furthermore, when it is considered that receiver apertures are parameterized with a finite length and power averaging needs to be considered, the power scintillation index σ 2 p is introduced. Its final equation is given in (9), where parameter d is calculated based in (10) [27].…”
Section: Atmospheric Turbulence Attenuation Based On Raob Databasementioning
confidence: 99%
See 1 more Smart Citation
“…Furthermore, when it is considered that receiver apertures are parameterized with a finite length and power averaging needs to be considered, the power scintillation index σ 2 p is introduced. Its final equation is given in (9), where parameter d is calculated based in (10) [27].…”
Section: Atmospheric Turbulence Attenuation Based On Raob Databasementioning
confidence: 99%
“…In order to compensate for the phase distortion, the reconstruction process is based on a deformable mirror controlled by a wave-front sensor. While the use of Shack-Hartmann wave sensor prevails within the last decade, its bandwidth limitations and saturation losses lead to the development of other early-stage technologies such as modal holographic wave-front sensors based on the Karhunen-Loève modes [9]. In addition, digital adaptive optics for turbulence mitigation is also considered [10].…”
Section: Introductionmentioning
confidence: 99%
“…More recent wavefront sensor developments include holographic and sensor-less techniques. 7 These systems compensate for turbulence in real time and use the full optical bandwidth of the receiving telescope. However, such systems still rely on reference source beacons in conjunction with deformable mirrors to physically apply the compensations and are thus generally expensive and complicated to operate.…”
Section: Introductionmentioning
confidence: 99%
“…A common AO method leverages a Shack–Hartmann 6 wavefront sensor; this device uses a microlens array to estimate phase aberrations. More recent wavefront sensor developments include holographic and sensor-less techniques 7 . These systems compensate for turbulence in real time and use the full optical bandwidth of the receiving telescope.…”
Section: Introductionmentioning
confidence: 99%
“…The most common wavefront sensor is a Shack-Hartmann 6 wavefront sensor, that utilizes a micro-lens array. More recent wavefront sensor developments include holography and sensor-less techniques 13 . These techniques still rely on using LASERS or some type of beacon as a reference source in conjunction with a deformable mirror to physically apply the compensation.…”
Section: Introductionmentioning
confidence: 99%