Performance analysis of adaptive-optics systems using laser guide stars and slope sensors

Physics – Optics

Scientific paper

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Adaptive Optics, Atmospheric Optics, Atmospheric Scattering, Laser Applications, Wave Front Reconstruction, Atmospheric Turbulence, Computer Techniques, Control Theory, Optical Transfer Function, White Noise

Scientific paper

Many current wave-front-reconstruction systems use localized phase-slope measurements to estimate wave fronts distorted by atmospheric turbulence. Analytical expressions giving the performance of this class of adaptive-optics system are derived. Performance measures include the mean-square residual phase error across the aperture, the optical transfer function, the point-spread function, and the Strehl ratio. For adaptive telescopes using laser guide stars, these measures can be used to determine the key design parameters for the laser.

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