• 센서학회지
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• 제7권1호
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• pp.39-44
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• 1998

연속적인 단일모드 광섬유에 설치 가능한 저반사율을 가진 광섬유 거울들이 기계식 접합기와 깨끗이 절단된 끝단면에 $TiO_{2}$ 유전체 물질로 코팅된 광섬유 단편들을 사용하여 만들어 졌다. 0.1%의 반사율을 가진 광섬유 거울들이 만들어 졌을 때 광섬유 거울의 삽입손실의 범위는 0.055dB 부터 0.3dB 였으며 평균 삽입손실은 0.15dB였다. 저반사율을 가진 광섬유 거울들은 필드에서 쉽게 만들어 질 수 있었다.

• 한국광학회:학술대회논문집
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• 한국광학회 2001년도 제12회 정기총회 및 01년도 동계학술발표회
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• pp.194-195
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• 2001

We fabricated fiber bragg gratings using interferometric method with Phase mask. The interferometer consisted of two plane-parallel mirrors and a phase mask perpendicular to mirrors. The Gratings were written using an Argon-ion laser. The experimental setup could change Bragg wavelength given by the phase mask. (omitted)

• 한국광학회지
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• 제34권1호
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• pp.22-30
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• 2023

조각거울은 우주용 관측위성의 주반사경을 크게 제작하기 위한 방법 중 하나로서, 여러 개의 작은 거울들을 이어 하나의 큰 거울로 이용하는 방법이다. 여러 개의 거울들을 하나의 거울로 정렬하기 위해서는 인접한 거울들 간에 기울기 오차(tilt)와 광축방향 정렬오차(piston)가 없어야 한다. 기울기 오차와 광축방향 정렬오차를 해결해야 여러 개의 거울이 한 방향으로 빛을 모으고, 이를 통해 뚜렷한 이미지를 얻을 수 있기 때문에 조각거울의 정렬오차를 나노미터 수준으로 측정할 수 있는 파면 센서가 필요하다. 기울기 오차는 조각거울을 통해 얻은 이미지를 통해 어떤 거울의 기울기가 틀어졌는지 쉽게 확인할 수 있는 반면, 광축방향 정렬오차는 이미지의 질은 떨어뜨리지만 드러나는 뚜렷한 특징이 없기 때문에 같은 방법으로 감지하기 어려워 세밀한 측정이 매우 중요하다. 이를 위해 본 논문에서는 지상용 초기 정렬시 많은 이점을 갖는 광학계 평가용 간섭계 중 하나인 피조 간섭계를 이용한다. 피조 간섭계를 사용한 복수 조각거울의 광축방향 정렬오차 측정을 위한 기초 연구로서 단일 조각거울의 광축방향 변위 오차를 측정하고, 측정불확도를 계산해서 피조 간섭계의 광축방향 변위 오차 측정 한계를 규명한다. 또한 수식을 통해 조각거울 광축방향 변위 오차와 간섭계로 측정한 표면 초점오차(defocus)의 관계를 계산했고, 도출한 수식의 타당성을 실험으로 검증했다.

• 천문학회보
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• 제40권2호
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• pp.40.1-40.1
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• 2015

Off-axis reflective optical systems have attractive advantages relative to their on-axis or refractive counterparts, for example, zero chromatic aberration, no obstruction, and a wide field of view. For the efficient operation of off-axis reflective system, the surface accuracy of freeform mirrors should be higher than the order of wavelengths at which the reflective optical systems operate. Especially for applications in shorter wavelength regions, such as visible and ultraviolet, higher surface accuracy of freeform mirrors is required to minimize the light scattering. In this work, we propose the error compensation algorithm (ECA) for the correction of wavefront errors on freeform mirrors. The ECA converts a form error pattern into polynomial expression by fitting a least square method. The error pattern is measured by using an ultra-high accurate 3-D profilometer (UA3P, Panasonic Corp.). The measured data are fitted by two fitting models: Sag (Delta Z) data model and form (Z) data model. To evaluate fitting accuracy of these models, we compared the fitted error patterns with the measured error pattern.

• Journal of Astronomy and Space Sciences
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• 제29권1호
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• pp.79-84
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• 2012

After a visit by Peter Waddell from the University of Strathclyde, Glasgow, UK in 1991, Robert H. Koch launched a program at the University of Pennsylvania to build lightweight pneumatic membrane mirrors, initially for balloon flight observations where weight is at a premium. Mirror cells were fabricated from sizes 0.18 m to 1.77 m, and experiments conducted to characterize the mirror figure and stability. Most of the work stopped after Prof. Koch's retirement in 1996 until 2006 when the authors expressed an interest in building an array of medium-aperture portable telescopes. The program restarted in earnest at Gravic, Inc. in Malvern, PA in 2008 with Koch using his extensive observational astronomy experience to guide the fabrication of a fully operational 1.07 m membrane mirror telescope with an optical tube assembly weighing under 45 Kg. Residual wavefront aberrations remediation resulted in Koch and the authors investigating membrane tensioning techniques with different cell designs, active secondary wavefront correction, photometric algorithms for aberrated images, and the use of additional lightweight mirror substrates from the Alt-Az Initiative Group, such as foamed glass. The best result for the lightweight mirrors was a point spread function spot size of several arc seconds. A lightweight 1.6 m cast aluminum cell alt-az telescope was subsequently designed by Koch and the authors for prime focus use.

• Journal of the Optical Society of Korea
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• 제13권2호
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• pp.178-183
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• 2009

At the time that the Keck-I 10m telescope was constructed in 1993, the era of Very Large Telescopes (VLTs) was opened. Now thirteen VLTs are in operation, and the largest of the monolithic mirrors is 8.4 m in diameter. Such monolithic mirrors are mostly aspheric and require high accuracies on the surface figures, reaching up to the diffraction limit. At present, next generation telescopes, Giant telescopes, are being developed. One is the GMT (Giant Magellan Telescope) whose size is 25.4 m in diameter. The primary mirror consists of seven segments figuring elliptical shapes on the surface. The surrounding six segments are off-axis and the edges are steep, as the fast focal ratio is adopted. It means that testing of the mirrors is a challenging task. In this paper, testing methods for the GMT primary mirror are reviewed, and accuracy of measuring devices is assessed. Results and discussions follow.

• 천문학논총
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• 제32권1호
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• pp.359-361
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• 2017

We report our research on aluminum mirror optics for future infrared astronomical satellites. For space infrared missions, cooling the whole instrument is crucial to suppress the infrared background and detector noise. In this aspect, aluminum is appropriate for cryogenic optics, because the same material can be used for the whole structure of the instrument including optical components thanks to its excellent machinability, which helps to mitigate optical misalignment at low temperatures. We have fabricated aluminum mirrors with ultra-precision machining and measured the wave front errors (WFEs) of the mirrors with a Fizeau interferometer. Based on the power spectral densities of the WFEs, we confirmed that the surface accuracy of all the mirrors satisfied the requirements for the SPICA Coronagraph Instrument. We then integrated the mirrors into an optical system, and examined the image quality of the system with an optical laser. As a result, the total WFE is estimated to be 33 nm (rms) from the Strehl ratio. This is consistent with the WFEs estimated from the measurement of the individual mirrors.

• 보존과학회지
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• 제37권6호
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• pp.767-777
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• 2021

본 연구는 전라남도 고흥과 담양지역에서 출토된 청동거울의 금속학적 분석으로 제작방법을 확인하고자 하였다. 연구한 대상 유물은 담양 제월리 고분에서 출토된 청동거울 2점, 고흥 봉룡리에서 발견된 청동거울 1점으로 총 3점이다. 분석 결과 X선을 이용한 조사에서 육안으로 관찰되지 않던 균열과 부식으로 인해 발생된 결실부와 주조제작으로 인해 형성된 기공을 확인할 수 있었다. 청동거울의 주성분은 Cu-Sn-Pb이며 Cu 73~79 wt%, Sn 17~21 wt%, Pb 3~4 wt%로 2 wt% 이상의 Pb이 포함되어 있어 청동거울에 필요한 주조성 및 기계적 성질을 조절하기 위한 것으로 확인된다. 또한 미세조직 관찰 결과 주조한 상태에서 추가적인 열처리가 이루어지지 않은 α상과 α+δ공석상의 조직으로 비교적 이른 시기에 제작된 삼국시대 청동거울로 추정할 수 있다.

• 한국정밀공학회지
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• 제17권4호
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• pp.129-134
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• 2000

This paper presents the development of ultra-precision machining process of large aspheric aluminum mirrors with a maximum diameter of 620 mm. An ultra-precision machine, "Nanoturn60", developed by Daewoo Heavy Industries Ltd. is used for machining and motion errors of the machine are compensated by using the FTS developed by IAE(Institue for Advanced Engineering) during the machining process. To check the form accuracy of machined aspheric surfaces, on-machine form measurement system is developed. This measurement system consists of air bearing touch probe, straight edge, and laser sensor. With in-process error compensation by FTS(Fast Tool Servo), aspheric mirrors with the from accuracy of submicron order are obtained. obtained.

• 한국정밀공학회지
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• 제15권12호
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• pp.169-179
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• 1998

Plane mirror type laser interferometers are popularly being used in many modern ultraprecision machines, as they can perform simultaneous measurements of multiple axis positions with nanometer resolution capabilities. One important issue in this application of laser interferometers is to provide a good level of alignment between the reflecting mirrors and the laser beams so that measurement errors due to undesirable coupling effects can be avoided in multiple axis measurements In this investigation, a thorough metrological analysis is given to develop an suitable mathematical model for a precision x-y stage in which the orthogonality misalignment between the reflecting mirrors significantly affects overall x-y mea-surement results. Then a noble calibration method is suggested in which two-dimensional displacement sensors of moire gratings of concentric circles are used to realize the reversal principle of orthogonality evaluation in situ. Finally, actual experimental results are discussed to verify that the suggested method can effectively calibrate the orthogonality error with an uncertainty of 0.2667 arcsec.