Paper
27 June 2006 The wavefront correction system for the Advanced Technology Solar Telescope
Author Affiliations +
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.
© (2006) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
T. Rimmele, K. Richards, J. M. Roche, S. L. Hegwer, R. P. Hubbard, E. R. Hansen, B. Goodrich, and R. S. Upton "The wavefront correction system for the Advanced Technology Solar Telescope", Proc. SPIE 6272, Advances in Adaptive Optics II, 627212 (27 June 2006); https://doi.org/10.1117/12.672330
Lens.org Logo
CITATIONS
Cited by 8 scholarly publications.
Advertisement
Advertisement
RIGHTS & PERMISSIONS
Get copyright permission  Get copyright permission on Copyright Marketplace
KEYWORDS
Adaptive optics

Wavefronts

Telescopes

Wavefront sensors

Control systems

Mirrors

Digital signal processing

RELATED CONTENT

W.M. Keck Observatory adaptive optics program
Proceedings of SPIE (May 31 1994)
Low-cost solar adaptive optics in the infrared
Proceedings of SPIE (February 11 2003)
The Giant Magellan Telescope phasing system
Proceedings of SPIE (September 13 2012)
PCR a PC based wave front reconstructor for MMT...
Proceedings of SPIE (July 14 2008)

Back to Top