Reconstruction of a Wavefront Distorted by Atmospheric Turbulence with Account for Optical Scheme of the Telescope

Reconstruction of a wavefront containing turbulent distortions of optical radiation is considered. The Hartmann method based reconstruction is carried out using the wave function approximation by Zernike polynomials according to estimates of local slopes and analyzed on the basis of filling Hartmann...

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Veröffentlicht in:Optoelectronics, instrumentation, and data processing instrumentation, and data processing, 2019-11, Vol.55 (6), p.631-637
Hauptverfasser: Kucherenko, M. A., Lavrinov, V. V., Lavrinova, L. N.
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Sprache:eng
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