Interpretation of out-of-focus star images in terms of wave-front curvature.

Details Interpretation of out-of-focus star images in terms of wave-front curvature. Interpretation of out-of-focus star images in terms of wave-front curvature.

Jan 1994

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1994josaa..11..425b&link_type=abstract

Journal of the Optical Society of America A, Vol. 11, No. 1, p. 425 - 427

Physics

Optics

Adaptive Optics

Scientific paper

The wave-front-curvature-sensing method used by F. Roddier for the University of Hawaii's curvature-adaptive-optics system is derived from the interpretation in 1979 of the out-of-focus images obtained by use of the Multiple Mirror Telescope. The author summarizes those original Multiple Mirror Telescope observations and the simple interpretation given in terms of wave-front curvature by use of geometrical optics at that time.

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