English

Fast & Furious focal-plane wavefront sensing

Instrumentation and Methods for Astrophysics 2015-06-19 v1 Optics

Abstract

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 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 x 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 x 320 pixels. The remaining wavefront rms error is estimated to be ~0.15 rad with FF and ~0.10 rad with FF-GS.

Keywords

Cite

@article{arxiv.1406.1006,
  title  = {Fast & Furious focal-plane wavefront sensing},
  author = {Visa Korkiakoski and Christoph U. Keller and Niek Doelman and Matthew Kenworthy and Gilles Otten and Michel Verhaegen},
  journal= {arXiv preprint arXiv:1406.1006},
  year   = {2015}
}

Comments

17 pages, 15 figures, accepted for publication in Applied Optics

R2 v1 2026-06-22T04:30:22.160Z