Hostname: page-component-cd9895bd7-q99xh Total loading time: 0 Render date: 2024-12-26T18:05:04.889Z Has data issue: false hasContentIssue false
  • English
  • Français

Prospects in Adaptive Optics for Solar Applications

Published online by Cambridge University Press:  03 August 2017

François Roddier  and
J. Elon Graves
François Roddier
Affiliation:
Institute for Astronomy, University of Hawaii at Manoa, 2680 Woodlawn Drive, Honolulu, HI 96822, U.S.A.
J. Elon Graves
Affiliation:
Institute for Astronomy, University of Hawaii at Manoa, 2680 Woodlawn Drive, Honolulu, HI 96822, U.S.A.

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

We review the theoretical perspective for problems in adaptive optics, outline recent progress, and consider its application in the infrared. Techniques in adaptive optics are on the threshold of revolutionizing modern astronomy. These techniques are particularly applicable in the infrared, where refractive effects of turbulence are reduced, characteristic cell sizes are greater, and the isoplanatic patch diameter is increased. Adaptive techniques could be especially appropriate for modern large solar telescopes now under consideration that could operate in the infrared.

Keywords

atmospheric effectsSun: generaltechniques: miscellaneoustelescopes
Type
Part 7: Infrared Technology and the Future
Information
Symposium - International Astronomical Union , Volume 154: Infrared Solar Physics , 1994 , pp. 557 - 566
Copyright
Copyright © Kluwer 1994 

References

Born, M. and Wolf, E.: 1975, Principles of Optics, Pergamon Press, New York, p. 464.Google Scholar
Chassat, F.: 1989, J. Opt. (Paris) 20, 13.CrossRefGoogle Scholar
Fried, D. L.: 1966, J. Opt. Soc. Am. 56, 1372.Google Scholar
Roddier, F., Northcott, M., and Graves, J. E.: 1991, Pub. Astron. Soc. Pac. 103, 131.Google Scholar
Roddier, N.: 1990, SPIE Conf. Proc. 1237, 668.Google Scholar