An iterative zonal wave-front estimation algorithm for slope or gradient-type data in optical testing acquired with regular or irregular pupil shapes is presented. In the mathematical model proposed, the optical surface, or wave-front shape estimation, which may have any pupil shape or size, shares a predefined wave-front estimation matrix that we establish. Owing to the finite pupil of the instrument, the challenge of wave front shape estimation in optical testing lies in large part in how to properly handle boundary conditions. The solution we propose is an efficient iterative process based on Gerchberg-type iterations. The proposed method is validated with data collected from a 15 × 15-grid Shack-Hartmann sensor built at the Nanjing Astr...
We discuss error propagation in the slope-based and the difference-based wavefront estimations. The ...
We present a new method for determining the complete set of patient-specific ocular parameters, incl...
Shack-Hartmann wavefront sensing in general requires careful registration of the reimaged telescope ...
An iterative zonal wave-front estimation algorithm for slope or gradient-type data in optical testin...
An iterative zonal wave-front estimation algorithm for slope or gradient-type data in optical testin...
A generalized numerical wave-front reconstruction method is proposed that is suitable for diversifie...
Optical testing in adverse environments, ophthalmology and applications where characterization by cu...
Iterative algorithm methods and systems for slope or gradient-type data is presented for wavefront z...
Optical images of astronomical objects viewed through ground-based telescopes are blurred by the at...
A new approach to wave-front sensing for adaptive optics systems is presented. The method, which exp...
Abstract: This letter presents a new modal technique that reconstructs a wavefront using iterative F...
International audienceThe use of Fourier methods in wave-front reconstruction can significantly redu...
We discuss error propagation in the slope-based and the difference-based wavefront estimations. The ...
International audienceRefraction-based imaging systems, used in wave tank facilities, provide measur...
In the coming decade, a new generation of extremely large-scale ground-based astronomical telescopes...
We discuss error propagation in the slope-based and the difference-based wavefront estimations. The ...
We present a new method for determining the complete set of patient-specific ocular parameters, incl...
Shack-Hartmann wavefront sensing in general requires careful registration of the reimaged telescope ...
An iterative zonal wave-front estimation algorithm for slope or gradient-type data in optical testin...
An iterative zonal wave-front estimation algorithm for slope or gradient-type data in optical testin...
A generalized numerical wave-front reconstruction method is proposed that is suitable for diversifie...
Optical testing in adverse environments, ophthalmology and applications where characterization by cu...
Iterative algorithm methods and systems for slope or gradient-type data is presented for wavefront z...
Optical images of astronomical objects viewed through ground-based telescopes are blurred by the at...
A new approach to wave-front sensing for adaptive optics systems is presented. The method, which exp...
Abstract: This letter presents a new modal technique that reconstructs a wavefront using iterative F...
International audienceThe use of Fourier methods in wave-front reconstruction can significantly redu...
We discuss error propagation in the slope-based and the difference-based wavefront estimations. The ...
International audienceRefraction-based imaging systems, used in wave tank facilities, provide measur...
In the coming decade, a new generation of extremely large-scale ground-based astronomical telescopes...
We discuss error propagation in the slope-based and the difference-based wavefront estimations. The ...
We present a new method for determining the complete set of patient-specific ocular parameters, incl...
Shack-Hartmann wavefront sensing in general requires careful registration of the reimaged telescope ...