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Sparse matrix wavefront reconstruction: simulations and experimentsAdaptive optics systems with Shack-Hartmann wavefront sensors require reconstruction of the atmospheric phase error from slope measurements, with every sensor in the array being used in the computation of each actuator command. This fully populated reconstruction matrix can result in a significant computational burden for adaptive optics systems with large numbers of actuators. A method for generating sparse wavefront reconstruction matrices for adaptive optics isproposed. The method exploits the relevance of nearby slope measurements for control of an individual actuator, and relies upon the limited extent of the influence function for a zonal deformable mirror. Relying only on nearby sensor information can significantly reduce the calculation time for wavefront reconstruction. In addition, a hierarchic controller is proposed to recover some of the global wavefront information. The performance of these sparse wavefront reconstruction matrices was evaluated in simulation, and tested on the Palomar Adaptive Optics System. This paper will present some initial results from the simulations and experiments.
Document ID
20210001318
Acquisition Source
Jet Propulsion Laboratory
Document Type
Other
External Source(s)
Authors
Dekany, R.
Burrus, R.
Brack, G.
Troy, M.
MacMartin, D.
Shi, F.
Date Acquired
August 22, 2002
Publication Date
August 22, 2002
Publication Information
Publisher: UNKNOWN
Distribution Limits
Public
Copyright
Other
Technical Review
Keywords
space
telescope
segmented
mirror
wavefront
sensing
and
control

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