In an adaptive optics (AO) system, noise and detection error can produce errors in the slope measurement of a Hartmann-Shack (HS) wavefront sensor and have further effects on the performance of the AO System. The noise in an AO system can be divided into the readout noise and the photon noise. The detection error in an AO system results from the discrete sampling by using number-limited CCD pixels in the HS sensor and the deadspace between the CCD pixels. A theoretical model for numerically simulating the effects of noise and detection error is presented and a corresponding computer program has been compiled, which is combined with our existing program of numerical simulation of the laser propagation in a turbulent media and an AO system in...
Characterizing an adaptive optics (AO) system refers to understanding its performance and limitation...
A comprehensive model of laser propagation in the atmosphere with a complete adaptive optics (AO) sy...
International audienceThe ultimate performance of adaptive optics is limited by the quality of the w...
It is well known that noise and detection error can affect the performances of an adaptive optics (A...
Wavefront sensors, which use solid-state CCD or CMOS photosensors, are sources of errors in adaptive...
The dynamic control process in an adaptive optics (AO) system is the third important factor to affec...
Aims. Adaptive optics (AO) system performance is improved using post-processing techniques, such as ...
A Shack-Hartmann (SH) wavefront sensor (WFS) is used in most modern adaptive optics systems where pr...
Modern adaptive optics systems represent a significantchallenge for automatic control. The output di...
Laser guide stars on an Extremely Large Telescope (ELT) produce elongated spots on the subapert...
We present the results of reduction of laser beam geometrical fluctuations that we have experimental...
Context. Adaptive optics (AO) is a technique allowing for ground-based telescopes’ angular resolutio...
The new generation of extremely large telescopes will have adaptive optics. Due to the complexity an...
Characterizing an adaptive optics (AO) system refers to understanding its performance and limitation...
A comprehensive model of laser propagation in the atmosphere with a complete adaptive optics (AO) sy...
International audienceThe ultimate performance of adaptive optics is limited by the quality of the w...
It is well known that noise and detection error can affect the performances of an adaptive optics (A...
Wavefront sensors, which use solid-state CCD or CMOS photosensors, are sources of errors in adaptive...
The dynamic control process in an adaptive optics (AO) system is the third important factor to affec...
Aims. Adaptive optics (AO) system performance is improved using post-processing techniques, such as ...
A Shack-Hartmann (SH) wavefront sensor (WFS) is used in most modern adaptive optics systems where pr...
Modern adaptive optics systems represent a significantchallenge for automatic control. The output di...
Laser guide stars on an Extremely Large Telescope (ELT) produce elongated spots on the subapert...
We present the results of reduction of laser beam geometrical fluctuations that we have experimental...
Context. Adaptive optics (AO) is a technique allowing for ground-based telescopes’ angular resolutio...
The new generation of extremely large telescopes will have adaptive optics. Due to the complexity an...
Characterizing an adaptive optics (AO) system refers to understanding its performance and limitation...
A comprehensive model of laser propagation in the atmosphere with a complete adaptive optics (AO) sy...
International audienceThe ultimate performance of adaptive optics is limited by the quality of the w...