Paper
11 July 2018 Tropospheric seeing effects on site selection and the use of adaptive optics for solar telescopes
Author Affiliations +
Abstract
Because of the very small size of the isoplanatic patch resulting from high altitude, tropopause seeing, the use of the Solar Differential Image Motion Monitor (S-DIMM) for solar seeing observations at large zenith distances is significantly compromised. I examine the resulting limitations and attempt to correct for these in its use for the Advanced Technology Solar Telescope (ATST/DKIST) site survey. Suggestions are given about how one might correct for this altitude seeing by Dual Conjugate and Multi-Conjugate Adaptive Optics (DCAO/MCAO). I also comment on adaptive optics for corona observations with the use of Laser Guide Star aided wavefront sensing.
© (2018) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Jacques Maurice Beckers "Tropospheric seeing effects on site selection and the use of adaptive optics for solar telescopes", Proc. SPIE 10703, Adaptive Optics Systems VI, 107036Y (11 July 2018); https://doi.org/10.1117/12.2304661
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KEYWORDS
Solar telescopes

Adaptive optics

Coronagraphy

Lanthanum

Observatories

Sun

Telescopes

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