Applied Optics · 2014 · 36 citations · 22 references
Natural SciencesPhysicsBiomedical OpticsOpticsVisual OpticsFourier OpticsLens SystemsOptical AberrationsSpherical AberrationWavefront-guided CorrectionError ReductionPupil ShapeSpatial Light ModulatorsStrehl RatioWavefront CorrectionWavefront Error EstimationWavefront ReconstructionWavefront Sensing
We present two complementary algorithms suitable for using focal-plane measurements to control a wavefront corrector with an extremely high-spatial resolution. The algorithms use linear approximations to iteratively minimize the aberrations seen by the focal-plane camera. The first algorithm, Fast & Furious (FF), uses a weak-aberration assumption and pupil symmetries to achieve fast wavefront reconstruction. The second algorithm, an extension to FF, can deal with an arbitrary pupil shape; it uses a Gerchberg-Saxton (GS)-style error reduction to determine the pupil amplitudes. Simulations and experimental results are shown for a spatial-light modulator controlling the wavefront with a resolution of 170×170 pixels. The algorithms increase the Strehl ratio from ∼0.75 to 0.98-0.99, and the intensity of the scattered light is reduced throughout the whole recorded image of 320×320 pixels. The remaining wavefront rms error is estimated to be ∼0.15 rad with FF and ∼0.10 rad with FF-GS.
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Phase retrieval algorithms: a comparison
James R. Fienup · Applied Optics · 1982 · 5.6K citations
The Structure of High Strehl Ratio Point‐Spread Functions
Marshall D. Perrin, Anand Sivaramakrishnan, Russell B. Makidon et al. · The Astrophysical Journal · 2003 · 144 citations · Full text
Natural Sciences, Astronomy, Physics +16