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EnglishIn this article we present a preliminary study and experimental results on the use of an adaptive optics (AO) system for the reduction of geometrical fluctuations in a laser beam. The AO system is based on a Shack–Hartmann wave front sensor and a micromachined deformable mirror as a corrective element. The aim of this work is to investigate the applicability of such technologies to improving wave front clean-up conditions in long baseline interferometric gravitational wave detection.
| Titolo: | Adaptive Optics approach for pre-filtering of geometrical fluctuations of the input laser beam of an interferometric gravitational waves detector |
| Autori: | |
| Data di pubblicazione: | 2003 |
| Rivista: | |
| Abstract: | In this article we present a preliminary study and experimental results on the use of an adaptive optics (AO) system for the reduction of geometrical fluctuations in a laser beam. The AO system is based on a Shack–Hartmann wave front sensor and a micromachined deformable mirror as a corrective element. The aim of this work is to investigate the applicability of such technologies to improving wave front clean-up conditions in long baseline interferometric gravitational wave detection. |
| Handle: | http://hdl.handle.net/11386/1064417 |
| Appare nelle tipologie: | 1.1.2 Articolo su rivista con ISSN |
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