• Title/Summary/Keyword: zernike coefficient

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According to the Wavelength, the Analysis of Individual Eye Model's Aberration Change (파장에 따른 개별모형안의 수차변화 분석)

  • Kim, Se-Jin;Lim, Hyeon-Seon;Kim, Bong-Hwan;Kouh, Jeong-Hwi
    • Journal of Korean Ophthalmic Optics Society
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    • v.13 no.3
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    • pp.61-64
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    • 2008
  • Purpose: The analysis of individual eye model designed from clinical demonstration about emmetropia shows that the aberration would be changed by the wave change. Method: The model on the basis of clinical demonstration of eye ball is designed in a form of having 4 refraction surfaces and a constant refractive index. We analyzed designed twelve individual eye model into aberrations changes, as giving changes Fraunhofer lines's six wavelengths. Result: About individual eye model, change in the wavelength of the wavefront aberrations analysis using the Zernike coefficient. This data indicate that the shorter wave is, the more defocus increases and the deviation value of spherical aberration and RMS are widened. Conclusion: As quantity of defocus according to result wavelength change is shorter and shorter, inclination which is similar twelve individual eye model is bigger and bigger and individual eye model majority of cases, little change, and change is shown in part individual eye model is a significant performance degradation can be raised.

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Study of the Analysis Method for the Aspherical Tolerance of a Korsch Telescope Using a Q Polynomial (Q-Polynomial을 이용한 Korsch 망원경의 비구면 공차 분석 방법 연구)

  • Jun, Won-Kyoun;Lee, Han-Yul;Lee, Sang-min;Kim, Ki-hwan;Park, Seung Han;Jung, Mee-Suk
    • Korean Journal of Optics and Photonics
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    • v.31 no.6
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    • pp.328-333
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    • 2020
  • In this paper, we study the analysis method for the aspherical tolerance of a Korsch telescope using a Q polynomial. It is important to analyze the tolerances for evaluating quality in high-precision fabrication of aspherical reflectors for high-resolution satellites. Thus we express the aspheric surface in terms of a Q polynomial in which each coefficient term is composed independently, and analyze the tolerance of a Korsch telescope. We also analyze the tolerance using Zernike fringe sag, which expresses the shape error of an aspherical mirror. By comparing the two results, we confirm that the Q-polynomial method can be used to analyze an aspherical mirror.

The Study of Wavefront Aberration Reconstruction for Optical System (광학계의 파면수차 재구성에 대한 연구)

  • Park, Seong-Jong;Ju, Seok-Hee;Kim, Sung-Gyun
    • Journal of Korean Ophthalmic Optics Society
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    • v.10 no.4
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    • pp.357-364
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    • 2005
  • To develope the assessment equpiments of an optical system using adaptive optics, we developed the program of wavefront reconstruction for an optical system like eye. We used matlab in order to program the wavefront reconstruction for an optical system and presented the wavefront function of optical system by the zemike polynomials using modal method. To test the developed program, we calculated the zemike coefficient(n=7) of cooke triplet using code V, and compared the wavefront shape and the zemike polynomials using code V to those using the developed program. In this case, the used zemike coefficients were n=2, 3, 4, 5, 6, 7, 8, 9, and 10 and the number of sub-aperture were 1,253. From these results, we know that the reconstructed wavefronts were similar to the wavefront of cooke triplet as n was the larger than 4 and the zemike coefficient was equal to that of cooke triplet as n was 7. The developed program is able to be applied to the core technology to develope the assessment equipment of an optical system using the adaptive optics.

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