By Vladimir P. Lukin, Boris V. Fortes
Because of the vast program of adaptive optical platforms, an figuring out of optical wave propagation in randomly inhomogeneous media has turn into crucial, and several other numerical versions of person AOS elements and of effective correction algorithms were built. This monograph includes precise descriptions of the mathematical experiments that have been designed and performed in the course of greater than a decade's worthy of research.
- Preface to the English variation
- Mathematical Simulation of Laser Beam Propagation within the surroundings
- Modeling an Adaptive Optics approach
- Adaptive Imaging
- Minimization and part Correction of Thermal Blooming of High-Power Beams
- A Reference Beacon as a Key component to an Adaptive Optics process
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Additional info for Adaptive Beaming and Imaging in the Turbulent Atmosphere (SPIE Press Monograph Vol. PM109)
R. D. Feit, “Time-dependent propagation of a highenergy laser beam through the atmosphere,” Appl. , 10, No. 1, pp. 129–139, 1976. P. I. Z Ser. , 24, No. 4, pp. 434–442, 1981. A. Konyaev, “Modification of the splitting method for numerical solution of quasi-optical problems,” in Abstracts of Reports at the VI Conference on Laser Beam Propagation in the Atmosphere, pp. 195–198, 1981. M. M. Flatte, “Intensity images and statistics from numerical simulation of wave propagation in 3-D random media,” Appl.
129–139, 1976. P. I. Z Ser. , 24, No. 4, pp. 434–442, 1981. A. Konyaev, “Modification of the splitting method for numerical solution of quasi-optical problems,” in Abstracts of Reports at the VI Conference on Laser Beam Propagation in the Atmosphere, pp. 195–198, 1981. M. M. Flatte, “Intensity images and statistics from numerical simulation of wave propagation in 3-D random media,” Appl. 11, pp. 2111–2126, 1988. V. Bykov, Numerical Simulation in Statistical Radiotechnics, Sov. Radio, Moscow, 1971.
2 it can be seen that linear and quadratic aberrations are affected considerably by the loss of spatial scales larger than the size of the computational grid. This fact is also confirmed by calculation of the variance for the coefficients of wavefront expansion in terms of the Zernike polynomials for turbulent spectral density with the finite outer scale. The parameter 1 , which characterizes phase distortions minus the phase constant over the entire aperture (polynomial Z1 ), is much less than the corresponding theoretical value.