We demonstrate the existence of higher-order curvature adaptive optics (AO) systems and compare their performance with the current 85-element system being built at the Institute for Astronomy at the University of Hawaii. Simulation results show that systems with in excess of 500 actuators are possible with actuator patterns that are simple extensions of the 85-element design. The attenuation of residual phase error within the Nyquist frequency of the deformable mirror (DM) satisfies the (-5/6) power law. A high-order system is also analyzed in which the pattern of wavefront sensor is synthesized from square pixels and the curvature actuators of the DM are also rectangular. The Strehl performance is ∼2% worse than its annular analog. © 2006 ...
The purpose of this study was to evaluate the performance of a bimorph deformable mirror from AOptix...
The use of adaptive optics (AO) in ground-based astronomy is be-coming increasingly mainstream. Whil...
Adaptive Optics (AO) can greatly enhance the resolution of astronomical images, achieving close to d...
This thesis describes computer simulations of a new wavefront sensing technique for Adaptive Optics ...
Adaptive optics (AO), as the technology of compensating the wavefront distortion can significantly i...
The refractive index of air varies a.o. with temperature, humidity, pressure and the CO2 concentrati...
A small amount of work has been done on this project; the strategy to be adopted has been better def...
Refractive index variations in the earth's atmosphere cause wavefront aberrations and limit thereby ...
We present a promising approach to the extremely fast sensing and correction of small wavefront erro...
The capability of the adaptive optics to correct for the segmentation error is analyzed in terms of ...
Compared with the conventional adaptive optics (AO) system, the sensorless AO system can greatly red...
A key component of any adaptive optics system (AO) for the correction of wavefront aberrations, is t...
Thanks to the availability of high actuator density deformable mirrors (ALPAO 468 DM), the high vers...
Deformable mirror is a widely used wavefront corrector in adaptive optics system, especially in astr...
The new generation of extremely large telescopes will have adaptive optics. Due to the complexity an...
The purpose of this study was to evaluate the performance of a bimorph deformable mirror from AOptix...
The use of adaptive optics (AO) in ground-based astronomy is be-coming increasingly mainstream. Whil...
Adaptive Optics (AO) can greatly enhance the resolution of astronomical images, achieving close to d...
This thesis describes computer simulations of a new wavefront sensing technique for Adaptive Optics ...
Adaptive optics (AO), as the technology of compensating the wavefront distortion can significantly i...
The refractive index of air varies a.o. with temperature, humidity, pressure and the CO2 concentrati...
A small amount of work has been done on this project; the strategy to be adopted has been better def...
Refractive index variations in the earth's atmosphere cause wavefront aberrations and limit thereby ...
We present a promising approach to the extremely fast sensing and correction of small wavefront erro...
The capability of the adaptive optics to correct for the segmentation error is analyzed in terms of ...
Compared with the conventional adaptive optics (AO) system, the sensorless AO system can greatly red...
A key component of any adaptive optics system (AO) for the correction of wavefront aberrations, is t...
Thanks to the availability of high actuator density deformable mirrors (ALPAO 468 DM), the high vers...
Deformable mirror is a widely used wavefront corrector in adaptive optics system, especially in astr...
The new generation of extremely large telescopes will have adaptive optics. Due to the complexity an...
The purpose of this study was to evaluate the performance of a bimorph deformable mirror from AOptix...
The use of adaptive optics (AO) in ground-based astronomy is be-coming increasingly mainstream. Whil...
Adaptive Optics (AO) can greatly enhance the resolution of astronomical images, achieving close to d...