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Optical Engineering

Expected performance of solar adaptive optics in large-aperture solar telescopes
Author(s): Jose Marino
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Paper Abstract

High resolution ground based solar observations require adaptive optics correction. The next generation of solar telescopes will have large aperture sizes, in the range of 4 m, and will require larger and more complex adaptive optics systems. We study the effects that extended field wavefront sensors have on the correction performance for large aperture size telescopes. These effects are more pronounced for observations at low elevation angles, which are common during high resolution solar observations. Additionally, atmospheric dispersion is strongest at low elevation angle observations and can cause further reductions of the adaptive optics performance. We present a study of the expected correction performance of solar adaptive optics systems in large-aperture solar telescopes using an end-to-end adaptive optics simulation package.

Paper Details

Date Published: 11 June 2012
PDF: 8 pages
Opt. Eng. 51(10) 101709 doi: 10.1117/1.OE.51.10.101709
Published in: Optical Engineering Volume 51, Issue 10
Show Author Affiliations
Jose Marino, National Solar Observatory (United States)


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