A novel wave-front sensor that estimates phase from Fourier intensity measurements is described, and an explicit expression is found and numerically evaluated for the Cramtr-Rao lower bound on integrated rms wave-front phase estimation error. For comparison, turbulence-aberrated wave-front phases and corresponding noisy Fourier intensity measurements were computer simulated. An iterative phase-retrieval algorithm was then used to estimate the phase from the Fourier intensity measurements and knowledge of the shape of an aperture through which the wave front passed. The simulation error approaches the lower bound asymptotically as the noise is reduced. 1
<p>Phase diversity wave-front sensing technique (PD) is a widely known estimation method of wave-fro...
Increasing interest in astronomical applications of non-linear curvature wavefront sensors for turbu...
Accurately extracting phase or phase derivative is the most important requirement in optical metrolo...
We apply a phase retrieval algorithm to the intensity pattern of a Hartmann wavefront sensor to meas...
A new approach to wave-front sensing for adaptive optics systems is presented. The method, which exp...
Thesis (Ph. D.)--University of Rochester. Institute of Optics, 2008.We apply phase retrieval, a meth...
International audienceWe introduce in this paper a general formalism for Fourier-based wave front se...
Optical images of astronomical objects viewed through ground-based telescopes are blurred by the at...
International audienceUsing Fourier methods to reconstruct the phase measured by a wavefront sensor ...
Recent studies of coherent wave propagation through turbulence have shown that under conditions wher...
Experimental results indicate that the statistics of phase measured across a telescope aperture do n...
International audienceIn this paper, we describe Fourier-based Wave Front Sensors (WFS) as linear in...
International audienceIn this paper, we describe Fourier-based Wave Front Sensors (WFS) as linear in...
We develop a phase reconstruction algorithm for the Shack–Hartmann wavefront sensor (SHWFS) that is ...
Under the scalar paraxial approximation, an optical wavefield is considered to be complex function d...
<p>Phase diversity wave-front sensing technique (PD) is a widely known estimation method of wave-fro...
Increasing interest in astronomical applications of non-linear curvature wavefront sensors for turbu...
Accurately extracting phase or phase derivative is the most important requirement in optical metrolo...
We apply a phase retrieval algorithm to the intensity pattern of a Hartmann wavefront sensor to meas...
A new approach to wave-front sensing for adaptive optics systems is presented. The method, which exp...
Thesis (Ph. D.)--University of Rochester. Institute of Optics, 2008.We apply phase retrieval, a meth...
International audienceWe introduce in this paper a general formalism for Fourier-based wave front se...
Optical images of astronomical objects viewed through ground-based telescopes are blurred by the at...
International audienceUsing Fourier methods to reconstruct the phase measured by a wavefront sensor ...
Recent studies of coherent wave propagation through turbulence have shown that under conditions wher...
Experimental results indicate that the statistics of phase measured across a telescope aperture do n...
International audienceIn this paper, we describe Fourier-based Wave Front Sensors (WFS) as linear in...
International audienceIn this paper, we describe Fourier-based Wave Front Sensors (WFS) as linear in...
We develop a phase reconstruction algorithm for the Shack–Hartmann wavefront sensor (SHWFS) that is ...
Under the scalar paraxial approximation, an optical wavefield is considered to be complex function d...
<p>Phase diversity wave-front sensing technique (PD) is a widely known estimation method of wave-fro...
Increasing interest in astronomical applications of non-linear curvature wavefront sensors for turbu...
Accurately extracting phase or phase derivative is the most important requirement in optical metrolo...