1. Date of download: 6/21/2016 Copyright © 2016 SPIE. All rights reserved. AO corrected average Strehl ratios at different field positions and Sun elevations at a wavelength of 550 nm. The FOV of the WFS is 0 arcsec and the global value of r0=10 cm. Figure Legend: From: Expected performance of solar adaptive optics in large-aperture solar telescopes Opt. Eng. 2012;51(10):101709-1-101709-7. doi:10.1117/1.OE.51.10.101709

2. Date of download: 6/21/2016 Copyright © 2016 SPIE. All rights reserved. Diagram showing sub-aperture images produced by a 10×10 cross-correlating Shack-Hartman WFS tracking on a sunspot. Each sub-image subtends a FOV of 20 arcsec. Figure Legend: From: Expected performance of solar adaptive optics in large-aperture solar telescopes Opt. Eng. 2012;51(10):101709-1-101709-7. doi:10.1117/1.OE.51.10.101709

3. Date of download: 6/21/2016 Copyright © 2016 SPIE. All rights reserved. AO corrected average Strehl ratios at different field positions and Sun elevations at a wavelength of 550 nm. The FOV of the WFS is 8 arcsec and the global value of r0=10 cm. Figure Legend: From: Expected performance of solar adaptive optics in large-aperture solar telescopes Opt. Eng. 2012;51(10):101709-1-101709-7. doi:10.1117/1.OE.51.10.101709

4. Date of download: 6/21/2016 Copyright © 2016 SPIE. All rights reserved. AO corrected average Strehl ratios at different field positions and Sun elevations at a wavelength of 550 nm. The FOV of the WFS is 16 arcsec and the global value of r0=10 cm. Figure Legend: From: Expected performance of solar adaptive optics in large-aperture solar telescopes Opt. Eng. 2012;51(10):101709-1-101709-7. doi:10.1117/1.OE.51.10.101709

5. Date of download: 6/21/2016 Copyright © 2016 SPIE. All rights reserved. Normalized AO corrected average Strehl ratios at different field positions for WFS FOV of 0, 8, and 16 arcsec and a Haleakala atmospheric profile. The wavelength is 550 nm and the global value of r0=10 cm. Figure Legend: From: Expected performance of solar adaptive optics in large-aperture solar telescopes Opt. Eng. 2012;51(10):101709-1-101709-7. doi:10.1117/1.OE.51.10.101709

6. Date of download: 6/21/2016 Copyright © 2016 SPIE. All rights reserved. AO corrected average Strehl ratios at different field positions and Sun elevations at a wavelength of 1600 nm. The FOV of the WFS is 16 arcsec and the global value of r0=10 cm. Figure Legend: From: Expected performance of solar adaptive optics in large-aperture solar telescopes Opt. Eng. 2012;51(10):101709-1-101709-7. doi:10.1117/1.OE.51.10.101709

7. Date of download: 6/21/2016 Copyright © 2016 SPIE. All rights reserved. Average AO corrected on-axis Strehl ratios at different Sun elevations for different observation and AO wavelengths. Symbols indicate the AO system operating at 500 nm. Lines without symbols indicate the AO system operating at the same wavelength as the observations. The FOV of the WFS is 0 arcsec and the global value of r0=10 cm. Figure Legend: From: Expected performance of solar adaptive optics in large-aperture solar telescopes Opt. Eng. 2012;51(10):101709-1-101709-7. doi:10.1117/1.OE.51.10.101709

8. Date of download: 6/21/2016 Copyright © 2016 SPIE. All rights reserved. Average AO corrected on-axis Strehl ratios at different Sun elevations for different observation and AO wavelengths. Symbols indicate the AO system operating at 500 nm. Lines without symbols indicate the AO system operating at the same wavelength as the observations. The FOV of the WFS is 16 arcsec and the global value of r0=10 cm. Figure Legend: From: Expected performance of solar adaptive optics in large-aperture solar telescopes Opt. Eng. 2012;51(10):101709-1-101709-7. doi:10.1117/1.OE.51.10.101709