This thesis describes computer simulations of a new wavefront sensing technique for Adaptive Optics based on local wavefront curvature measurements, along with edge slope measurements. The output signal from the curvature measurements, along with edge slope measurements. The output signal from the curvature sensor can be directly applied to the electrodes of a bimorph or membrane mirror. The mirror is used as an analog device to solve the Poisson Equation, providing a fast real time compensation for atmospheric disturbances. The open loop characteristics of the system are presented. The ideal response is analyzed, and side effects such as non-linearity, photon and diffraction noises are discussed. Closed loop simulations are presented there...
Adaptive Optics is a technics allowing for the correction in real-time of the evoluting and non-pred...
Atmospheric turbulence limits the resolving power of astronomical telescopes by distorting the path...
One major disadvantage to ground based observations is the distortion of light as it enters the Eart...
The applicability of wave-front correction by means of a bimorph mirror in conjunction with a curvat...
This research outlines the development and simulation of a signal processing approach to real time w...
We demonstrate the existence of higher-order curvature adaptive optics (AO) systems and compare thei...
A small amount of work has been done on this project; the strategy to be adopted has been better def...
While developing deformable mirrors for adaptive optics, and while studying scintillation, we also t...
Shack-Hartmann (SH) sensor, based on sampling of wavefront tilts in subapertures, is a simple, relia...
Optical images of astronomical objects viewed through ground-based telescopes are blurred by the at...
We consider the Neumann boundary-value problem for curvature adaptive optics systems. We show that, ...
In this paper, a wavefront curvature sensor is presented. This sensor is based on the measurements o...
Adaptive optics increases the angular resolution of large, ground-based telescopes by compensating ...
Adaptive optics systems with Shack-Hartmann wavefront sensors require reconstruction of the atmosphe...
The use of adaptive optics (AO) in ground-based astronomy is be-coming increasingly mainstream. Whil...
Adaptive Optics is a technics allowing for the correction in real-time of the evoluting and non-pred...
Atmospheric turbulence limits the resolving power of astronomical telescopes by distorting the path...
One major disadvantage to ground based observations is the distortion of light as it enters the Eart...
The applicability of wave-front correction by means of a bimorph mirror in conjunction with a curvat...
This research outlines the development and simulation of a signal processing approach to real time w...
We demonstrate the existence of higher-order curvature adaptive optics (AO) systems and compare thei...
A small amount of work has been done on this project; the strategy to be adopted has been better def...
While developing deformable mirrors for adaptive optics, and while studying scintillation, we also t...
Shack-Hartmann (SH) sensor, based on sampling of wavefront tilts in subapertures, is a simple, relia...
Optical images of astronomical objects viewed through ground-based telescopes are blurred by the at...
We consider the Neumann boundary-value problem for curvature adaptive optics systems. We show that, ...
In this paper, a wavefront curvature sensor is presented. This sensor is based on the measurements o...
Adaptive optics increases the angular resolution of large, ground-based telescopes by compensating ...
Adaptive optics systems with Shack-Hartmann wavefront sensors require reconstruction of the atmosphe...
The use of adaptive optics (AO) in ground-based astronomy is be-coming increasingly mainstream. Whil...
Adaptive Optics is a technics allowing for the correction in real-time of the evoluting and non-pred...
Atmospheric turbulence limits the resolving power of astronomical telescopes by distorting the path...
One major disadvantage to ground based observations is the distortion of light as it enters the Eart...