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- W2005694819 abstract "By employing the geometric OTF, the author proposes a criterion to determine the axial best image point of an optical system having spherical aberration. The criterion is expressed by Sigma j=1N(J1(2 pi nu TA*(rj))rj tan psi ), where nu signifies the spatial frequency, TA* means the aberration, rj denotes the pupil radius, and psi is the function of the f/stop of the system. A numerical example is also added to illustrate the analysis." @default.
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- W2005694819 date "1985-09-01" @default.
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- W2005694819 title "The best image criterion based on geometric OTF for optical systems with spherical aberration" @default.
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- W2005694819 doi "https://doi.org/10.1088/0150-536x/16/5/002" @default.
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