We present an adaptive optics approach to improve the image quality of telescopes observing targets through atmospheric turbulences. Intended as an enhancement for off-the-shelf imaging systems an f/10 achromatic lens telescope is expanded by relay telescopes and dichroitic beam splitters to satisfy the adaptive optics requirements. A high speed Shack-Hartmann wavefront sensor and an adaptive membrane mirror are located in conjugated planes. A non-deterministic PC system provides a fast closed-loop frequency of 500 Hz. The system characteristics are investigated and first results in terms of wavefront diagrams and resolution charts are presented
International audienceThe ultimate performance of adaptive optics is limited by the quality of the w...
Epigrams on Programming, Alan J Perlis Abstra t Atmospheric turbulence limits the resolving power of...
Modern ground-based telescopes rely on Adaptive Optics (AO) systems, which compensate for atmospheri...
Several studies on different adaptive optics concepts are presented in the article. Each one of the ...
High-resolution telescope systems used for observational tasks require sufficiently large apertures ...
Abstract. Observations with ground based telescopes suffer from atmospheric turbulence. Inde-pendent...
Observations of fainter and fainter astrophysical objects in the universe require an increasing flux...
Severely Iimited by atmospheric turbulence, large ground based telescopes are not capable of attaini...
We present a promising approach to the extremely fast sensing and correction of small wavefront erro...
Atmospheric turbulence limits the resolving power of astronomical telescopes by distorting the path...
Adaptive Optics (AO) is a key technology for ground-based astronomical telescopes, allowing to overc...
Compensation of extended (deep) turbulence effects is one of the most challenging problems in adapti...
Abstract. The wavefront aberrations induced by atmospheric turbulence can severely degrade the perfo...
(Member) date AFIT/GE/ENG/09-33 Adaptive optics applies advanced sensing and control to improve the ...
Technological advances and the ever-growing human quest for improving the resolution of telescope ob...
International audienceThe ultimate performance of adaptive optics is limited by the quality of the w...
Epigrams on Programming, Alan J Perlis Abstra t Atmospheric turbulence limits the resolving power of...
Modern ground-based telescopes rely on Adaptive Optics (AO) systems, which compensate for atmospheri...
Several studies on different adaptive optics concepts are presented in the article. Each one of the ...
High-resolution telescope systems used for observational tasks require sufficiently large apertures ...
Abstract. Observations with ground based telescopes suffer from atmospheric turbulence. Inde-pendent...
Observations of fainter and fainter astrophysical objects in the universe require an increasing flux...
Severely Iimited by atmospheric turbulence, large ground based telescopes are not capable of attaini...
We present a promising approach to the extremely fast sensing and correction of small wavefront erro...
Atmospheric turbulence limits the resolving power of astronomical telescopes by distorting the path...
Adaptive Optics (AO) is a key technology for ground-based astronomical telescopes, allowing to overc...
Compensation of extended (deep) turbulence effects is one of the most challenging problems in adapti...
Abstract. The wavefront aberrations induced by atmospheric turbulence can severely degrade the perfo...
(Member) date AFIT/GE/ENG/09-33 Adaptive optics applies advanced sensing and control to improve the ...
Technological advances and the ever-growing human quest for improving the resolution of telescope ob...
International audienceThe ultimate performance of adaptive optics is limited by the quality of the w...
Epigrams on Programming, Alan J Perlis Abstra t Atmospheric turbulence limits the resolving power of...
Modern ground-based telescopes rely on Adaptive Optics (AO) systems, which compensate for atmospheri...