• 제목/요약/키워드: Optical Mirror

검색결과 759건 처리시간 0.02초

루프 미러로 구성된 기준팔을 가지는 파장 스위핑 OCT 구현 (Realization of Swept Source Optical Coherence Tomography with Loop Mirror Reference Arm)

  • 김훈섭;남궁명우;이정렬;엄진섭
    • 산업기술연구
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    • 제27권B호
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    • pp.121-123
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    • 2007
  • As a reflector of reference arm in OCT systems, a coated fiber reflector has mostly used. Instead, this paper has realized the swaept source optical coherence tomography system using a loop mirror within a reference arm. Through the experiments for a tilted thin glass plate, we found that the loop mirror is better than the coated fiber typed mirror for obtaining the clear image.

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A Nickel Micro Switch Operating in a Wide Range of Torsion Angles

  • Kahng, Seong-Joong;Kim, Jae-Hyeok;Kim, Young-Min
    • Journal of Electrical Engineering and Technology
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    • 제2권2호
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    • pp.263-266
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    • 2007
  • We report a nickel optical MEMS switch, being able to rotate through a large angle and to accommodate multiple channels. The proposed optical switch consists of a thin nickel mirror and two torsion springs supporting the mirror. The torsion springs are designed using a finite element method (FEM) such that plastic deformation of the thin nickel is avoided during the large torsion actuation. For switching speed improvement, transient vibration of the released mirror is suppressed by optimizing the mirror design and a fast switching response of $200\;{\mu}s\;(pull-down)/300\;{\mu}s\;(pull-up)$ is demonstrated.

Performance Improvement of Near Earth Space Survey (NESS) Wide-Field Telescope (NESS-2) Optics

  • Yu, Sung-Yeol;Yi, Hyun-Su;Lee, Jae-Hyeob;Yim, Hong-Suh;Choi, Young-Jun;Yang, Ho-Soon;Lee, Yun-Woo;Moon, Hong-Kyu;Byun, Yong-Ik;Han, Won-Yong
    • Journal of Astronomy and Space Sciences
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    • 제27권2호
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    • pp.153-160
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    • 2010
  • We modified the optical system of 500 mm wide-field telescope of which point spread function showed an irregularity. The telescope has been operated for Near Earth Space Survey (NESS) located at Siding Spring Observatory (SSO) in Australia, and the optical system was brought back to Korea in January 2008. After performing a numerical simulation with the tested value of surface figure error of the primary mirror using optical design program, we found that the surface figure error of the mirror should be fabricated less than root mean square (RMS) $\lambda$/10 in order to obtain a stellar full width at half maximum (FWHM) below $28\;{\mu}m$. However, we started to figure the mirror for the target value of RMS $\lambda$/20, because system surface figure error would be increased by the error induced by the optical axis adjustment, mirror cell installation, and others. The radius of curvature of the primary mirror was 1,946 mm after the correction. Its measured surface figure error was less than RMS $\lambda$/20 on the table of polishing machine, and RMS $\lambda$/15 after installation in the primary mirror cell. A test observation performed at Daeduk Observatory at Korea Astronomy and Space Science Institute by utilizing the exiting mount, and resulted in $39.8\;{\mu}m$ of stellar FWHM. It was larger than the value from numerical simulation, and showed wing-shaped stellar image. It turned out that the measured-curvature of the secondary mirror, 1,820 mm, was not the same as the designed one, 1,795.977 mm. We fabricated the secondary mirror to the designed value, and finally obtained a stellar FWHM of $27\;{\mu}m$ after re-installation of the optical system into SSO NESS Observatory in Australia.

레이저 재료 가공을 위한 광폭빔 광학 장치 (Wide Beam Optical System for the Laser Materials Processing)

  • 김재도;조응산;전병철
    • 한국레이저가공학회지
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    • 제1권1호
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    • pp.24-29
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    • 1998
  • A new wide laser beam optical system for the laser materials processing has been developed with a polygonal mirror. It consists of polygonal mirror and cooling part that prevents the surface of rotating polygonal mirror from damage by heat. The polygonal minors have been designed and made as 24 and 30 facets in pyramid type. This system provides a uniform linear laser heat source with the surface scanning width from 15 to 50mm according to the scanning height To examine the wide laser beam, He-Ne laser is used. Also, Acryl is used to confirm the laser beam pattern by bum-pattern print To analyze the energy distribution of the wide laser ben empirical values and theoretical values are compared and discussed. To improve the efficiency of the wide laser beam optical system, methods are suggested by the optical theories. For larger area processing like turbine blade, drawing blade, cold roller and guide plate, optimal overlapping locations have been calculated and analyzed by geometric and optical theories.

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반응표면법을 이용한 광학미러용 일체형 유연힌지 마운트 최적설계 (Optimal Design of the Monolithic Flexure Mount for Optical Mirror Using Response Surface Method)

  • 이경호;남병욱;남성식
    • 한국군사과학기술학회지
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    • 제26권3호
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    • pp.205-213
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    • 2023
  • An optimal design of a simple beam-shaped flexure hinge mount supporting an optical mirror is presented. An optical mirror assembly is an opto-mechanically coupled system as the optical and mechanical behaviors interact. This side-supporting mount is flexible in the radial direction and rigid for the remaining degrees of freedom to support the mirror without transferring thermal load. Through thermo-elastic, optical and eigenvalue analysis, opto-mechanical performance was predicted to establish the objective functions for optimization. The key design parameters for this flexure are the thickness and length. To find the optimal values of design parameters, response surface analysis was performed using the design of experiment based on nested FCD. Optimal design candidates were derived from the response surface analysis, and the optimal design shape was confirmed through Opto-mechanical performance validation analysis.

Beer-Lambert 법칙을 적용한 레이저 열원 프로파일 모델링 및 레이저무기용 반사경의 열변형 해석을 통한 구조-열-광학 성능 연구 (A Study on Structural-Thermal-Optical Performance through Laser Heat Source Profile Modeling Using Beer-Lambert's Law and Thermal Deformation Analysis of the Mirror for Laser Weapon System)

  • 홍대기
    • 항공우주시스템공학회지
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    • 제17권4호
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    • pp.18-27
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    • 2023
  • 본 논문에서는 열해석의 하중조건으로 레이저 열원을 설정하여 반사경의 구조-열-광학 성능 분석을 수행하였다. 레이저 열원 모델은 가우시안 빔을 바탕으로 반투명한 소재를 고려한 Beer-Lambert 법칙을 적용하여 하중조건으로 선정하였으며, 반사경만의 성능 분석을 위하여 기구부는 고려하지 않았다. 열변형해석을 수행하여 반사경 표면의 온도 변화로 인한 열응력과 열변형 데이터를 얻었다. 열변형에 의한 반사경 표면의 변위 데이터를 Zernike 다항식에 피팅하여 파면오차를 계산하였으며, 이를 통해 고에너지 레이저가 반사경으로 입사될 때 반사경의 광학 성능을 예측할 수 있었다.

위상 공액 거울에 흡착된 분자의 광학적 성질 (Optical Properties of Admolecules near a Phase -Conjugate Mirror)

  • 김영식
    • 한국진공학회지
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    • 제5권1호
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    • pp.33-38
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    • 1996
  • The induced linewidth, frequency shift and absorption spectrum for a molecular dipole in the vicinity of a phase -conjugate mirror have been investgated within a classical phenomenological model, with particularreference to the technique of optical phase conjugation by a surface. While the shifts and the widths show similar characteristics as those obtained recently by Bochove who considered the problem within the context of four-wave mixing, the results obtained in the present model can be defined uniquely with the possibility of an infinite lifetime for the excited admolecule . Furthermore, the absorption lineshape obtained here some interesting features which depend on both the magnitude and the phase of the complex reflectivity of the mirror.

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대구경 반사경 광학성능 측정을 위한 간섭계 지지구조물의 진동저감 설계 (Vibration Suppression Design on the Instrument Supporting Structure for the Optical Performance Measurement)

  • 김홍배;임종민;양호순
    • 한국소음진동공학회:학술대회논문집
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    • 한국소음진동공학회 2005년도 추계학술대회논문집
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    • pp.205-208
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    • 2005
  • Fabrication of large scaled mirror for the telescope application is the most challenging technology in recent year. Sophisticate technologies and know-how in fabrication and measurement are required to overcome the technological obstacles. KRISS(Korea Research Institute for Standards and Science) is now developing a large scaled mirror fabrication facility and KARI(Korea Aerospace Research Institute) is supporting the development. High precision interferometric test is required during the grinding and polishing of mirror to identify the surface profile precisely. The required fabrication accuracy of the mirror surface profile is $\lambda$/50 ms($\sim$10 nm for visible wave length). Thus the measurement accuracy should be far less than 10 m. To get this requirement, it is necessary to provide vibration free environment for the interferometer system and mirror under test. Thus the vibration responses on the mirror supporting table due to external vibration should be minimized by using a special isolation system. And the responses on the top of the tower, which hold the interferometer during test, should be minimized simultaneously. In this paper, we propose the concept design of vibration suppression system for the KRISS mirror fabrication facility.

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타원면경 측정 Null 렌즈 설계 (Null lens design for testing of elliptical surface)

  • 김연수
    • 한국광학회지
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    • 제11권4호
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    • pp.246-249
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    • 2000
  • 고해상도 원격관측용 카메라오 설계된 비축 3반사 광학계의 제3거울인 타원면(원추계수>0) 형상측정 Null 렌즈를 설계하였다. Null 렌즈 설계방식으로는 측정감도는 2배로 높으면서 작은 기준 평면경을 사용하는 혼합방식을 제안하였다. 혼합방식과 autostigmatic 방식으로 설계한 Null 렌즈의 광파면 왜곡 민감도를 비교하여 혼합방식이 보다 유리한 Null 측정 광학게임을 제시하였다.

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Integral-floating Display with 360 Degree Horizontal Viewing Angle

  • Erdenebat, Munkh-Uchral;Baasantseren, Ganbat;Kim, Nam;Kwon, Ki-Chul;Byeon, Jina;Yoo, Kwan-Hee;Park, Jae-Hyeung
    • Journal of the Optical Society of Korea
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    • 제16권4호
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    • pp.365-371
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    • 2012
  • A three-dimensional integral-floating display with 360 degree horizontal viewing angle is proposed. A lens array integrates two-dimensional elemental images projected by a digital micro-mirror device, reconstructing three-dimensional images. The three-dimensional images are then relayed to a mirror via double floating lenses. The mirror rotates in synchronization with the digital micro-mirror device to direct the relayed three-dimensional images to corresponding horizontal directions. By combining integral imaging and the rotating mirror scheme, the proposed method displays full-parallax three-dimensional images with 360 degree horizontal viewing angle.