Paper
28 July 2010 Adaptive optics system for the IRSOL solar observatory
Renzo Ramelli, Roberto Bucher, Leopoldo Rossini, Michele Bianda, Silvano Balemi
Author Affiliations +
Abstract
We present a low cost adaptive optics system developed for the solar observatory at Istituto Ricerche Solari Locarno (IRSOL), Switzerland. The Shack-Hartmann Wavefront Sensor is based on a Dalsa CCD camera with 256 pixels × 256 pixels working at 1kHz. The wavefront compensation is obtained by a deformable mirror with 37 actuators and a Tip-Tilt mirror. A real time control software has been developed on a RTAI-Linux PC. Scicos/Scilab based software has been realized for an online analysis of the system behavior. The software is completely open source.
© (2010) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Renzo Ramelli, Roberto Bucher, Leopoldo Rossini, Michele Bianda, and Silvano Balemi "Adaptive optics system for the IRSOL solar observatory", Proc. SPIE 7736, Adaptive Optics Systems II, 77363K (28 July 2010); https://doi.org/10.1117/12.857160
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Cited by 1 scholarly publication.
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KEYWORDS
Adaptive optics

Mirrors

Cameras

Wavefronts

Wavefront sensors

Observatories

Spectrographs

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