Two-sided pyramid wavefront sensor in the direct phase mode

Proceedings of SPIE - The International Society for Optical Engineering

Volumn 6272 II, Issue , 2006, Pages

  Phillion, Donald W ^a   Baker, Kevin ^a  

^a LAWRENCE LIVERMORE NATIONAL LABORATORY   (United States)

Author keywords

Adaptive optics; Pyramid wavefront sensor

Indexed keywords

FOURIER SPACE; HILBERT TRANSFORM; PHASE VARIATION; PYRAMID WAVEFRONT SENSOR;

ADAPTIVE OPTICS; ATMOSPHERIC TURBULENCE; CLOSED LOOP CONTROL SYSTEMS; COMPUTER SIMULATION; ITERATIVE METHODS; SPACE OPTICS; SPECKLE;

OPTICAL SENSORS;

EID: 33749424455     PISSN: 0277786X     EISSN: None     Source Type: Conference Proceeding    
DOI: 10.1117/12.671961     Document Type: Conference Paper

References (6)

1. Robert Ragazzoni, "Pupil plane wave sensing with an oscillating prism", J. Mod. Opt. 43 No. 2, 1996. pp 289-293
2. C. Verinaud, "On the nature of the measurements provided by a pyramid wave-front sensor", Opt. Comm. 233, 2004, pp 27-38
3. Olivier Guyon, "Limits of Adaptive Optics for high contrast imaging", Astrophys. J. 629 (2005) pp 592-614
4. C. Verinaud, M. Le Louarn, V. Korkiakoski, and M. Carbillet, "Adaptive Optics for high-contrast imaging pyramid sensor versus spatially filtered Shack-Hartmann sensor", Mon. Not. R. Astron. Soc. 357, L26-L30, 2005.
5. The Telescope AO code is written in Microsoft Visual C++ and requires Windows XP Professional. It has the pyramid WFS simulator and can be obtained from phillionl@llnl.gov
6. Matthew C. Brirton, "Arroyo", Proc. of SPIE Vol. 5497 (SPIE, Bellingham, WA, 2004), pp 290-300