In this paper we investigate the performance of a Fourier based algorithm for fast subpixel shift determination of two mutually shifted images subjected to noise. The algorithm will be used for Shack-Hartmann based adaptive optics correction of images of an extended object subjected to dynamical atmospheric fluctuations. The performance of the algorithm is investigated both analytically and by Monte Carlo simulations. Good agreement is achieved in relation to how the precision of the shift estimate depends on image parameters such as contrast, photon counts and readout noise, as well as the dependence on sampling format, zero-padding and field of view. Compared to the conventional method for extended object wavefront sensing, a reduction of...
An important factor which affects performance of solar adaptive optics (AO) systems is the accuracy ...
Because atmospheric turbulence causes distortions in stellar wavefronts, passive ground based telesc...
The atmosphere introduces a phase distortion on the incoming wavefront from an astronomical object, ...
We present an adaptive periodic-correlation algorithm for large dynamic range extended-scene Shack-H...
Adaptive Periodic-Correlation (APC) algorithm was developed for use in extended-scene Shack-Hartmann...
International audienceThe ultimate performance of adaptive optics is limited by the quality of the w...
Optical images of astronomical objects viewed through ground-based telescopes are blurred by the at...
We present a promising approach to the extremely fast sensing and correction of small wavefront erro...
The turbulent atmosphere degrades images of objects viewed through it by introducing random amplitud...
Without any form of compensation, atmospheric turbulence blurs the images obtained by ground-based t...
We investigate methods to calibrate the non-common path aberrations at an adaptive optics system hav...
Correlation wave-front sensing can improve Adaptive Optics (AO) system performance in two keys areas...
Context. Solar Shack–Hartmann wavefront sensors measure differential wavefront tilts as th...
Wavefront sensor is designed to measure both intensity distribution and phase distortion of optical ...
Phase aberrations in optical systems,which occur in various applications such as astronomy, microsco...
An important factor which affects performance of solar adaptive optics (AO) systems is the accuracy ...
Because atmospheric turbulence causes distortions in stellar wavefronts, passive ground based telesc...
The atmosphere introduces a phase distortion on the incoming wavefront from an astronomical object, ...
We present an adaptive periodic-correlation algorithm for large dynamic range extended-scene Shack-H...
Adaptive Periodic-Correlation (APC) algorithm was developed for use in extended-scene Shack-Hartmann...
International audienceThe ultimate performance of adaptive optics is limited by the quality of the w...
Optical images of astronomical objects viewed through ground-based telescopes are blurred by the at...
We present a promising approach to the extremely fast sensing and correction of small wavefront erro...
The turbulent atmosphere degrades images of objects viewed through it by introducing random amplitud...
Without any form of compensation, atmospheric turbulence blurs the images obtained by ground-based t...
We investigate methods to calibrate the non-common path aberrations at an adaptive optics system hav...
Correlation wave-front sensing can improve Adaptive Optics (AO) system performance in two keys areas...
Context. Solar Shack–Hartmann wavefront sensors measure differential wavefront tilts as th...
Wavefront sensor is designed to measure both intensity distribution and phase distortion of optical ...
Phase aberrations in optical systems,which occur in various applications such as astronomy, microsco...
An important factor which affects performance of solar adaptive optics (AO) systems is the accuracy ...
Because atmospheric turbulence causes distortions in stellar wavefronts, passive ground based telesc...
The atmosphere introduces a phase distortion on the incoming wavefront from an astronomical object, ...