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Applied Optics

Applied Optics


  • Editor: Joseph N. Mait
  • Vol. 49, Iss. 10 — Apr. 1, 2010
  • pp: 1818–1825

Optical transfer functions derived from solar adaptive optics system data

Friedrich Wöger  »View Author Affiliations

Applied Optics, Vol. 49, Issue 10, pp. 1818-1825 (2010)

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Adaptive optics (AO) systems installed at large ground-based telescopes partially correct Earth’s atmosphere, making post facto image reconstruction techniques necessary to produce diffraction-limited observations. To achieve accurate photometry in the reconstructed images, some post facto techniques require knowledge of transfer functions that describe the optical system. I present a new, fast method for the estimation of the long-exposure and speckle transfer functions from data gathered by a solar AO system simultaneously with the observations. The results of the presented method are tested with extensive analytical models, demonstrating that the estimation is robust for situations where the AO system is performing with Strehl ratios larger than 45%. Application to observations of solar granulation produces reconstructed images that are photometrically in agreement with earlier results.

© 2010 Optical Society of America

OCIS Codes
(010.1290) Atmospheric and oceanic optics : Atmospheric optics
(010.1330) Atmospheric and oceanic optics : Atmospheric turbulence

ToC Category:
Atmospheric and Oceanic Optics

Original Manuscript: October 22, 2009
Revised Manuscript: January 27, 2010
Manuscript Accepted: February 19, 2010
Published: March 25, 2010

Friedrich Wöger, "Optical transfer functions derived from solar adaptive optics system data," Appl. Opt. 49, 1818-1825 (2010)

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