Wave-front sensing from artificial beacons is normally performed by formation of a focused spot in the atmosphere and sensing of the wave-front distortions produced during the beam's return passage. We propose an alternative method that senses the distortions produced during the outgoing path by forming an intensity pattern in the atmosphere that is then viewed from the ground. A key advantage of this method is that a parallel beam is used, and therefore the wave-front measurements will not suffer from the effects of focal anisoplanatism. We also envisage other geometries, all based on the concept of projecting a pupil pattern onto the atmosphere
© 2016 IEEE. The task of delivering sufficient level of airborne laser energy to ground based target...
The field of adaptive optics (AO) and laser-beacon AO has been successfully implemented in the last ...
Laser Guide Stars aim at increasing the sky coverage, highly restricted when using Adaptive Opt...
A method for producing a laser guide star wavefront sensor for adaptive optics with reduced focal an...
We have analysed and simulated a novel alternative Laser Guide Star (LGS) configuration termed Proje...
For the next generation of extremely large telescopes, Focal Anisoplanatism (FA) renders single Lase...
Focus anisoplanatism is a significant measurement error when using one single laser guide star (LGS)...
A dynamically ranged pulsed Rayleigh beacon using sensed wavefronts across a system’s pupil plane is...
The task of delivering sufficient level of airborne laser energy to ground based targets is of high ...
The problem of providing Adaptive Optics (AO) correction over a wide field of view is one that can b...
We address the problem of using adaptive optics to deliver power from an airborne laser platform to ...
We report on a high-resolution wave-front sensor that measures the complete spatial profile of any f...
We describe two new methods of using a laser guide star for wavefront sensing in order to reduce the...
Extending adaptive optics to laser beam control over long turbulent paths where there is no cooperat...
There is strong interest in developing adaptive optics solutions for extreme conditions, such as las...
© 2016 IEEE. The task of delivering sufficient level of airborne laser energy to ground based target...
The field of adaptive optics (AO) and laser-beacon AO has been successfully implemented in the last ...
Laser Guide Stars aim at increasing the sky coverage, highly restricted when using Adaptive Opt...
A method for producing a laser guide star wavefront sensor for adaptive optics with reduced focal an...
We have analysed and simulated a novel alternative Laser Guide Star (LGS) configuration termed Proje...
For the next generation of extremely large telescopes, Focal Anisoplanatism (FA) renders single Lase...
Focus anisoplanatism is a significant measurement error when using one single laser guide star (LGS)...
A dynamically ranged pulsed Rayleigh beacon using sensed wavefronts across a system’s pupil plane is...
The task of delivering sufficient level of airborne laser energy to ground based targets is of high ...
The problem of providing Adaptive Optics (AO) correction over a wide field of view is one that can b...
We address the problem of using adaptive optics to deliver power from an airborne laser platform to ...
We report on a high-resolution wave-front sensor that measures the complete spatial profile of any f...
We describe two new methods of using a laser guide star for wavefront sensing in order to reduce the...
Extending adaptive optics to laser beam control over long turbulent paths where there is no cooperat...
There is strong interest in developing adaptive optics solutions for extreme conditions, such as las...
© 2016 IEEE. The task of delivering sufficient level of airborne laser energy to ground based target...
The field of adaptive optics (AO) and laser-beacon AO has been successfully implemented in the last ...
Laser Guide Stars aim at increasing the sky coverage, highly restricted when using Adaptive Opt...