• 제어로봇시스템학회논문지
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• 제19권12호
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• pp.1089-1093
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• 2013

Depth extraction using the structured illumination method is popularly applied since it has the benefit of measuring the object without contact. With multiple spatial frequencies and phase-shifting techniques, it is possible to extract the depth of objects with large discontinuity. For applications such as 3D (Three Dimensional) displays, 3D information of the object is required and is useful if corresponding to each view of the display. For this purpose, hypercentric optics is appropriate to measure the depth information of an object with a large field of view that is applicable for a 3D display. By experiment, we present the feasibility for phase-shifting profilometry using hypercentric optics to obtain the depth information of an object with the field of view appropriate for a 3D display.

• 한국광학회지
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• 제16권1호
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• pp.71-78
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• 2005

대형 비구면의 측정을 위하여 자동무수차점 방식의 2매 구성 널 렌즈를 설계하였고, 제작과 정렬 오차에 따른 측정 정밀도의 한계를 이론적으로 분석해 보았다. 측정 정밀도의 한계를 결정짓는 주요한 공차 요소는 널 렌즈면의 불규칙도(irregularity)임을 확인하였으며, 불규칙도의 가공 정도에 따라 5λ/100∼4λ/1000 정도까지의 신뢰할 수 있는 측정 정밀도가 한정지어졌다. 이로써 실제의 정렬 오차 및 널 렌즈 제작오차까지 고려하여 신뢰할 수 있는 정밀도 한계를 제시할 수 있었다.

• Journal of the Optical Society of Korea
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• 제18권3호
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• pp.244-250
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• 2014

Due to the difficulty in measuring very low out-of-band cutoff depths of solar blind UV filters, we propose a cutoff depth adjustable measurement system (CDAM) to test deep cutoff filters with a large dynamic range. The CDAM utilizing the substitution method is elaborately composed of several parts, including narrow-band LED light sources, standard reflective neutral attenuators with known attenuation coefficients, and a photomultiplier (PMT). This paper also presents an attenuator combination method ensuring that the PMT works within its linear response range. In addition, numerical simulation testifies to the method, and experiment shows that the CDAM system can achieve an extension of dynamic range from 0-6 OD to 0-10 OD, which is sufficient for the measurement of out-of-band cutoff depths of solar blind UV filters. Above all, the CDAM system, being easily implemented, of wide dynamic range, and highly precise, could be widely used in the measurement of filter cutoff depth.

• 한국광학회:학술대회논문집
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• 한국광학회 2000년도 하계학술발표회
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• pp.3-3
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• 2000

Adaptive Optical (AO) technology can compensate for wave-front errors in real-time to improve image and beam quality. The research and development on AO in China began in 1979. In 1980, the first laboratory on AO in China was established in Institute of Optics and Electronics (IOE), Chinese Academy of Sciences (CAS). Since then several AO systems have been built in this Laboratory. The 19-element system is the first AO system in the world ever used in inertial confinement fusion (ICF) facility in our knowledge. It corrects the static error of this large laser engineering. The 21-element system was firstly tested at the 1.2m telescope of Kunming Observatory in 1990 and then up-dated as an IR AO system installed at the 2.16m telescope of Beijing Observatory. The 37-element system was used with a turbulence cell in Laboratory on Atmospheric Optics in Hefei to conduct elementary research on Atmospheric Optics. The 61-element system for astronomical observation is newly developed. It has been successfully installed at the 1.2m telescope of Kunming Observatory and a laser guide star system will be integrated with the system. A compact AO system using our newly developed miniature DM for high resolution ophthalmic imaging of retina is also being built. The key elements of these AO systems, deformable mirrors and fast-steering mirrors, are all developed in this Laboratory. In this talk, the main configurations of these AO systems, some test results as well as the specifications of these active mirrors will be presented.

• 한국정밀공학회지
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• 제30권3호
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• pp.324-330
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• 2013

This paper describes a novel method to surface large optics mirror with an extremely high hardness, which could replace the high cost of the repetitive off-line measurement steps and the large ultra-precision grinding machine with ultra-positioning control of 10 nm resolution. A lot of diamond pellet to be attached on the convex aluminum base consists of a grinding tool for the concave large mirror, and the tool was pressured down on the large mirror blank. The tool motion at an interval on the spiral path was controlled with each feed rate as the dwell time in the conventional computer-controlled polishing. The shape to be surfaced was measured directly by a touch probe on the machine without any separation of the mirror blank. Total 40 iterative steps of the surfacing and measurement could demonstrate the form error of RMS $7.8{\mu}m$, surface roughness of Ra $0.2{\mu}m$ for the mirror blank with diameter of 1 m and spherical radius of curvature of 5400 mm.

• 한국광학회:학술대회논문집
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• 한국광학회 2002년도 하계학술발표회
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• pp.24-25
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• 2002

밀레니움을 전후하여 세계적으로 8m급 초대형 망원경들이 만들어지고 있다. ESO (European Southern Observatory)의 VLT (Very Large Telescopes) 4기, 미국 영국 카나다 등의 연합 Gemini telescope 2기, 일본의 Subaru 1기 등, 10여기의 망원경들이 완성되었고, 차세대 망원경들이 50m급으로 디자인되고 있다. 우주망원경도 지름 2.4m인 허블 우주망원경(Nubble Space Telescope)의 뒤를 이어 6m급의 차세대 우주망원경 (Next Generation Space Telescope)이 개발되고 있어서 2010년경에 발사될 예정이다. (중략)

• Journal of the Optical Society of Korea
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• 제5권3호
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• pp.70-75
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• 2001

Next Generation Space Telescope (NGST) is under design study for proposed launch around 2008. It will take over the task of Hubble Space Telescope (HST) and provide much more detailed information about celestial objects. Present large telescopes both in space and on the ground contain aspheric mirrors, called Ritchey-Chretien type. As the size of the telescope becomes larger and the optical quality is requested to be higher, reaching the diffraction limit, more accurate optical testing methods are required. However, there are few testing methods which can achieve the required accuracy for aspheric optics, and none of them has achieved it with certainty. The failure of producing the primary mirror of the Hubble Space Telescope to meet specification is a good example. Moreover, testing aspheric mirrors of large convex form adds the difficulty to extreme. In this paper, space telescopes and large ground-based telescopes are surveyed and testing methods for aspheric optics are reviewed. a method of testing aspheric convex mirrors is suggested.

• 한국전자파학회논문지
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• 제21권11호
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• pp.1240-1247
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• 2010

본 논문은 한반도 지역에 개인 휴대 단말을 사용한 보편적 통신 방송 서비스를 제공하기 위한 S-대역 위성 탑재용 다중 빔 대형 안테나의 전기적 설계 방법에 대해 연구한 것이다. 배열 소자로 급전되는 반사판 형태인 하이브리드 안테나로 다중 빔을 구현하고, 각 빔은 급전 배열의 일부를 사용하여 형성된다. 원하는 빔을 얻기 위해서는 각 배열 소자 신호의 크기와 위상을 최적화해야 하고, 이는 GO(Geometrical Optics) 및 PO(Physical Optics) 해석을 통해 이루어졌다. 또한, EIRP(Effective Isotropically Radiated Power) 요구 사항을 만족하도록 배열 소자의 개수를 최적하였다. 위성에 탑재 가능하도록 제한된 크기의 반사판을 사용하고, 배열 소자의 개수를 최소화하면서도 요구 사항을 만족시킬 수 있는 설계 방법과 그 성능 결과를 본 논문에서 확인할 수 있을 것이다.

• Journal of the Optical Society of Korea
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• 제16권4호
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• pp.457-461
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• 2012

A real-time method to measure full field retardation near quarter wavelength is proposed. The circularly polarized beam passes through a sample with a large aperture. The measuring beam then goes through a quarter-wave plate and is then split by a Wollaston prism. An image with two sub-images is then detected by a high-speed image sensor. The full field retardation near quarter wavelength can be obtained in real time by processing the image. The measured retardation is independent of the fast axis angle of the sample and the fluctuation of the initial intensity. In experiments, a wedge waveplate is measured with different fast axis angle and initial intensity, and the full field retardations are acquired. The maximum and standard deviation of the full field retardation is $1.5^{\circ}$ and $0.4^{\circ}$. The validity of the method is verified.

• 한국안광학회지
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• 제5권1호
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• pp.199-203
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• 2000

콘택트렌즈 표면의 미세한 흠집이나 뜯김 등의 흠과 콘택트렌즈 edge부분의 연마상태나 파손여부를 식별하기 위해서는 배율이 커야하며, 또한 왜곡수차와 색수차가 제거되어야만 한다. 본 연구에 사용된 콘택트렌즈 분석기 "CONTACT LENS ANALYZER CA-20"은 표면검사에 적합한 16배의 큰 배율과 왜곡수차가 우선 제거된 우수한 분석기라고 말할 수 있다.