• Korean Journal of Optics and Photonics
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• v.17 no.4
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• pp.359-365
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• 2006

Wave-front error(WFE) is the main parameter that determines the optical performance of the opto-mechanical system. In the development of opto-mechanics, WFE due to the main loading conditions are set to the important specifications. The deformation of the optical surface can be exactly calculated thanks to the evolution of numerical methods such as the finite element method(FEM). To calculate WFE from the deformation results of FEM, another approximation of the optical surface deformation is required. It needs to construct additional grid or element mesh. To construct additional mesh is troublesomeand leads to transformation error. In this work, the moving least-squares approximation is used to reconstruct wave front error It has the advantage of accurate approximation with only nodal data. There is no need to construct additional mesh for approximation. The proposed method is applied to the examples of GOCI scan mirror in various loading conditions. The validity is demonstrated through examples.

• Journal of Astronomy and Space Sciences
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• v.17 no.1
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• pp.67-76
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• 2000

Far-ultraviolet IMaging Spectrograph(FIMS) is the main payload of the first Korean scientific satellite, KAISTSTA-4, which will be launched in 2002. The optical system of FIMS consists of parabolic cylinder mirror, slit, ellipsoidal reflection grating, and MCP to get spatial information as well as spectral information. Allowed ranges of manufacturing and positioning error are derived for each optical components to achieve the astronomical goals. In the procedure, graphical simplification is dedicated to understand sensitivity table and to derive range and precision of manipulation for each optical component. The result shows that precision of ${\mu}m$ for linear and of 2' for angular manipulation fulfills optical requirements.

• Proceedings of the Optical Society of Korea Conference
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• 2003.07a
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• pp.154-155
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• 2003

PMP(Phase Measuring Profilometry)측정법은 투영계와 기록계의 기하학적 구성과 광학계의 정렬적인 문제에 의해서 기본적으로 오차를 가지고 측정된다. 일반적으로 PMP 형상 측정에서 측정면과 광학계의 높이가 피 측정면에 비해서 상당히 큰 경우, CCD 카메라에서 높이 방향으로 측정영역이 작아지게됨으로써 측정위상이 기준면에서의 위치와 높이 방향에 따라서 다르게 나타나고 프로젝터가 측정면에 투영되는 간섭무의의 피치가 다르게 적용된다. (중략)

• Korean Journal of Remote Sensing
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• v.29 no.5
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• pp.555-568
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• 2013

Atmospheric optical thickness during nighttime was estimated in this study using analysis on the images of the moon taken from commercial digital camera. Basically the Langely Regression method was applied to the observations of the moon for the cloudless and optically stable sky conditions. The spectral response functions for the red(R), green(G), and blue(B) channels were employed to derive effective wavelength centers of each channel for the observations of the moon, and the correspondent Rayleigh optical thickness were also calculated. Aerosol optical thickness (AOT) was calculated by subtracting Rayleigh optical thickness from the atmospheric optical thickness derived from the Langley regression method. As there are only handful of nighttime AOT observations, the AOT from the moon observations was compared with the AOT from sun-photometers and the MODIS satellite sensor, which was taken several hours before the moon observations of this study. As a result, the values of AOT from moon observations agree with those from sun-photometers and MODIS within 0.1 for the R, G, B channels of the digital camera. On the other hand, ${\AA}$ngstr$\ddot{o}$m Exponent seems to be subject to larger errors due to its sensitiveness to the spectral errors of AOT. Nevertheless, the results of this study indicate that the method reported in this study is promising as it can provide nighttime AOT relatively easily with a low cost instrument like digital camera. More observations and analyses are warranted to attain improved nighttime AOT observations in the future.

• Korean Journal of Optics and Photonics
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• v.25 no.1
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• pp.29-37
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• 2014

We have studied and demonstrated general, systematic error-correction methods for a dual rotating quarter-wave plate ellipsometer. To estimate and correct 5 systematic error sources (three offset angles and two unexpected retarder phase delays), we used 11 of the 25 Fourier components of the ellipsometry signal obtained in the absence of an optical sample. Using these 11 Fourier components, we can determine the errors from the 5 sources with nonlinear optimization methods. We found systematic errors ${\epsilon}_3$, ${\epsilon}_4$, ${\epsilon}_5$) are more sensitive to the inverted Mueller matrix than retarder phase delay errors (${\epsilon}_1$, ${\epsilon}_2$) because of their small condition numbers. To correct these systematic errors we have found that error of any variety must be less than 0.05 rad. Finally, we can use the magnitudes of these errors to correct the Mueller matrix of optical components. From our experimental ellipsometry signals, we can measure phase delay and the rotational angular position of its fast axis for a half-wave plate.

• Proceedings of the Korean Institute of IIIuminating and Electrical Installation Engineers Conference
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• 2006.05a
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• pp.142-147
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• 2006

소자가 발광하는 형태를 가지며 매우 작은 크기의 광원인 LED는 특유의 형태 때문에 자체의 발광특성을 점광원으로 가정하여 부가적인 광학제품들이 설계되어 왔다. 하지만, 실제적인 설계에서는 이러한 점광원으로의 가정에서 오차를 불러일으킬 수 있으며, 세밀한 제어를 요구하는 조명시스템의 제어에서는 작은 오차라 해도 큰 에러를 발생시킬 수 있다. 따라서 본 논문에서는 점광원이 아닌 실제적인 부피를 지니는 광원으로서의 LED를 분석하여 그에 대한 2차적인 광학 시스템의 설계법을 제시하고자한다.

• Proceedings of the Optical Society of Korea Conference
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• 2003.02a
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• pp.90-91
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• 2003

대부분의 가공기 혹은 측정기에 있어 이송테이블은 그 기능수행의 기본을 담당하고 있으며 이송테이블의 운동 정밀도와 고속화는 목표하는 정밀도와 생산성으로 직결된다. 종래에는 형상특성, 열변형 등의 계통 오차만을 오프라인(Off-line)으로 측정하고 소프트웨어적으로 보상하는 방법을 사용하였으나 초정밀 분야에서 요구되는 테이블의 운동정밀도는 기계적 강성한계를 넘는 정밀도이므로, 테이블 이송 시 발생하는 운동오차를 실시간으로 측정하고, 보상할 수 있는 온라인(On-line)개념의 능동형 보상이 필요하다. (중략)

• Korean Journal of Optics and Photonics
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• v.12 no.5
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• pp.362-370
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• 2001

We prove that 3-D profile mapping using white light interferometry has systematic errors caused by aberrations of the optimal system. The tilt of an object invokes an offset between the object and the reference ray, which eventually makes the aberration cancel incompletely. The fringe peak of a white light interferogram is mainly affected by the aberration effect while the envelope peak remains stable. By the difference between the two peaks, it is easily confirmed how much the error existed in the fringe peak. Experimental results prove that the error caused by aberration is varied by object tilt, microscope NA, optics alignment within the range of $\pm$50nm.

• Proceedings of the Optical Society of Korea Conference
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• 2003.07a
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• pp.124-125
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• 2003

레이저 광선이 발명이 된 이래로 레이저 빔을 360도 전 방향으로 발사시키는 광학적 장치의 필요성이 매우 컸으며, 이를 이용한 응용장치가 많이 있다. 그러나, 불행히도 이제까지 레이저 빔을 360도 전 방향으로 발사시키는 광학적인 단일 요소가 개발된 적이 없었다. 이 레이저 빔을 360도 전 방향으로 발사시키는 광학적 장치는 회전거울 혹은 회전 홀로그램을 이용한 것이 고작이었다. 하지만, 이러한 회전식장치는 장치의 복잡성, 회전 모터의 회전축의 오차 등 여러 가지 불편한 점이나, 유지보수의 어려움 등을 가지고 있었다. (중략)

• Journal of the Korean Society of Surveying, Geodesy, Photogrammetry and Cartography
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• v.35 no.3
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• pp.125-132
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• 2017

Even after applying an image registration, Very High Resolution (VHR) multi-temporal images acquired from different optical satellite sensors such as IKONOS, QuickBird, and Kompsat-2 show a local misalignment due to dissimilarities in sensor properties and acquisition conditions. As the local misalignment, also referred to as Registration Noise (RN), is likely to have a negative impact on multi-temporal information extraction, detecting and reducing the RN can improve the multi-temporal image processing performance. In this paper, an approach to fine registration between VHR multi-temporal images by considering local distribution of RN is proposed. Since the dominant RN mainly exists along boundaries of objects, we use edge information in high frequency regions to identify it. In order to validate the proposed approach, datasets are built from VHR multi-temporal images acquired by optical satellite sensors. Both qualitative and quantitative assessments confirm the effectiveness of the proposed RN-based fine registration approach compared to the manual registration.