pith. sign in

arxiv: 1310.1241 · v1 · pith:TUVWI6TNnew · submitted 2013-10-03 · 🌌 astro-ph.IM · physics.optics

Calibrating a high-resolution wavefront corrector with a static focal-plane camera

classification 🌌 astro-ph.IM physics.optics
keywords wavefrontcorrectorcamerafocal-planehigh-resolutionlocatedmethodplane
0
0 comments X
read the original abstract

We present a method to calibrate a high-resolution wavefront-correcting device with a single, static camera, located in the focal plane; no moving of any component is needed. The method is based on a localized diversity and differential optical transfer functions (dOTF) to compute both the phase and amplitude in the pupil plane located upstream of the last imaging optics. An experiment with a spatial light modulator shows that the calibration is sufficient to robustly operate a focal-plane wavefront sensing algorithm controlling a wavefront corrector with ~40 000 degrees of freedom. We estimate that the locations of identical wavefront corrector elements are determined with a spatial resolution of 0.3% compared to the pupil diameter.

This paper has not been read by Pith yet.

discussion (0)

Sign in with ORCID, Apple, or X to comment. Anyone can read and Pith papers without signing in.