Abstract
For an optical system with a large amount of aberration, a merit function ∫ ∫A M (s,ψ) g(s) sd sdψ is proposed, where M(s,ψ) is a relative modulation function introduced by Hopkins, g(s) is a weighting function, and A denotes a circular region in the spatial frequency domain (s,ψ). It is shown that the above quantity can be expressed as a quadratic form of the aberration coefficients by using an appropriate approximation. As a numerical example, we set g(s) = 1 and calculate the coefficients of the quadratic terms of the wave-front aberrations.
© 1971 Optical Society of America
Full Article | PDF ArticleMore Like This
William B. King
J. Opt. Soc. Am. 59(9) 1155-1158 (1969)
Paul N. Robb
J. Opt. Soc. Am. 66(10) 1037-1041 (1976)
William B. King
J. Opt. Soc. Am. 62(2) 230-233 (1972)