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Proceedings Paper

The wavefront correction system for the Advanced Technology Solar Telescope
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Paper Abstract

An important part of a large solar telescope is the ability to correct, in real time, optical alignment errors caused by gravitational bending of the telescope structure and wavefront errors caused by atmospheric seeing. The National Solar Observatory is currently designing the 4 meter Advanced Technology Solar Telescope (ATST). The ATST wavefront correction system, described in this paper, will incorporate a number of interacting wavefront control systems to provide diffraction limited imaging performance. We will describe these systems and summarize the interaction between the various sub-systems and present results of performance modeling.

Paper Details

Date Published: 27 June 2006
PDF: 12 pages
Proc. SPIE 6272, Advances in Adaptive Optics II, 627212 (27 June 2006); doi: 10.1117/12.672330
Show Author Affiliations
T. Rimmele, National Solar Observatory (United States)
K. Richards, National Solar Observatory (United States)
J. M. Roche, Univ. of Alabama in Huntsville (United States)
S. L. Hegwer, National Solar Observatory (United States)
R. P. Hubbard, National Solar Observatory (United States)
E. R. Hansen, National Solar Observatory (United States)
B. Goodrich, National Solar Observatory (United States)
R. S. Upton, National Optical Astronomy Observatory (United States)

Published in SPIE Proceedings Vol. 6272:
Advances in Adaptive Optics II
Brent L. Ellerbroek; Domenico Bonaccini Calia, Editor(s)

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