• Korean Journal of Optics and Photonics
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• v.8 no.4
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• pp.260-266
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• 1997

Holographic optical elements for polarization separation (HPS) are fabricated in a dichromated gelatin(DCG) thin film of 7${\mu}{\textrm}{m}$ thickness. The polarization properties of HPS is characterized by measuring diffraction efficiency with several physical parameters like exposure time, incident angle and read-out polarization angles. The experimental data are compared with theoretical results based on Kogelnik's coupled wave theory, which shows good agreement. It is also found that the HPS element has a very high extinction ratio of polarization over 500:1 for S and P polarizations, respectively, with He-Ne laser wavelength. We also propose an optical switch optical interconnects by using HPS elements.

• Korean Journal of Optics and Photonics
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• v.15 no.1
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• pp.6-11
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• 2004

The playback wavelength shift and the optical property stabilization of the reflection type photopolymer OmniDex film are studied as a function of pressure. As the center wavelength is changed from 632 nm to 482 nm, the bandwidth is 27％ broadened and the diffraction efficiency deviation maintained lower than 10％. These results show that the proposed color tuning method minimizes the change of optical properties more than 50％ compared with the diffusion-based method as the center wavelength changed from 511 nm to 630 nm. The press-based color tuning method shows that it could be used to make holographic optical elements that operate at wavelengths where lasers are not readily available for reflection type holographic recording.

• Proceedings of the Optical Society of Korea Conference
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• 2009.02a
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• pp.371-372
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• 2009

• The Bulletin of The Korean Astronomical Society
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• v.35 no.1
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• pp.35.2-35.2
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• 2010

한국천문연구원은 미국 BBSO(Big Bear Solar Observatory)에 건설 중인 1.6 m NST(New Solar Telescope) 개발사업에 참여하고 있다. 고속태양영상분광기, FISS(Fast Imaging Solar Spectrograph)는 한국천문연구원과 서울대학교가 공동으로 개발하는 태양관측용 영상분광기로서, Echelle 회절격자를 분광소자로 사용하고 있다. FISS는 빠른 영상 스캐닝과 고속 CCD 카메라를 이용하여 동시에 두 파장을 관측할 수 있으며, NST의 적응광학계로부터 영상을 입력받기 때문에 회절한계에 가까운 분광영상을 얻을 수 있다. 본 연구에서는 FISS 제작을 위한 요구사항 분석, 분광기 구성과 광학설계, 구성품의 제작, 그리고 분광기의 성능검증을 위한 태양 시험관측 결과에 대해 소개한다.

• The Journal of Korean Institute of Communications and Information Sciences
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• v.17 no.12
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• pp.1353-1361
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• 1992

Holographic optical element(HOE) is fabricated with the properties of lightweight, thin thickness and interconnectivity for free space. Particularly, HOE for optical interconnection and multiple image processing should have a high efficiency and equal spot intensity, Nonlinear equations for 2-dimensional binary phase grating(BPG) structure is solved by computer simulation based on modified Newton method. Computer-generated pattern drawn by plotter is scaled down and translated into the microfilm. After contact printing between the microfilm and silver halide hologram film, phase diffraction grating produces the $5{\times}5$ multiple spots. Experimental results are shown that bleached phase grating has a high efficiency and equal focused beams except central zero order.

• Journal of the Korea Academia-Industrial cooperation Society
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• v.11 no.9
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• pp.3435-3440
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• 2010

Unlike the electric method capable of checking only product defect, the real time optical metrology is suggested for measuring and visualizing vibration with respect to position of surface acoustic wave in RF device. The measuring limits and conditions for surface acoustic wave is given, and the interference and diffraction due to RF signal are analyzed by optical interpretation. A single mode laser and a 105MHz-center-frequency repeater filter were employed for experiments and theoretical analysis. In this paper, the optical metrology providing visual energy distribution and real time inspection for surface acoustic wave is proposed for development of high quality multi-service and multi-frequency RF module.

• Journal of the Korean Institute of Telematics and Electronics D
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• v.35D no.6
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• pp.63-71
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• 1998

In this paper, we experiment the characteristics of coupling coefficient, gain, diffraction efficiency and dependence of time determined by TWM(Two-Wave Mixing), using Fe-LiNbO$_3$ crystal(doped with 0.015Wt.%). From these results, we proposed to apply for optical memory application. The highest coupling angle of 14。 and maximum coupling coefficient of 6.9$cm^{-1}$ / are obtained at 514.5nm wavelength. Also, maximum diffraction efficiency is 54.13% when intensity ratio and writing beam incident angle are 0.1 and 14o, respectively. After fixing process, diffraction efficiency is 21.4%. As an example, we demonstrated the writing and reconstruct optical data using spatial light modualtor and angular multiplexing in most optimal condition.

• Proceedings of the Materials Research Society of Korea Conference
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• 2003.03a
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• pp.95-95
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• 2003

최근, 대면적 평판표시소자 제작을 위한 전기발광 (EL; electroluminescence)소자용 소재로서 GaN 분말을 적용하고자 하는 연구가 진행되고 있다. 이와 같이 GaN 분말을 EL 소재로 사용하기 위해서는 원하는 파장의 빛을 발광할 수 있도록 특정의 불순물을 첨가하여야 할 필요가 있다. Mg이 첨가된 GaN 분말의 합성과 특성에 대한 연구가 있었으며, 희토류 원소가 첨가된 GaN 분말의 특성이 보고된바 있다. 본 논문에서는 GaOOH 분말을 출발물질로 채택하여 Zn가 첨가된 GaN 분말을 합성하고 광학적인 특성을 조사하였다. Zn가 첨가된 GaN 분말을 합성하기 위하여, 우선 CaOOH 분말 1g과 일정량의 ZnO 또는 Zn(NO$_3$)$_3$를 함께 섞어 유발에서 습식 혼합한 후 건조시켰다. Ga에 대한 Zn의 몰 비는 0.1부터 30 까지 변화시켰다. 반응온도는 900~110$0^{\circ}C$의 범위에서 변화시켰고, 반응시간은 1~4시간 범위에서 변화시켰으며, NH$_3$의 유량은 400 sccm으로 하였다. X선 회절분석장치를 사용하여 결정구조를 확인하였고, Zn의 첨가에 따른 광학적 특성은 10 K의 온도에서 광루미네센스(PL; photoluminescence)를 측정하여 평가하였다.

• Korean Journal of Optics and Photonics
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• v.5 no.2
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• pp.304-310
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• 1994

The use of thermally expanded core (TEe) fibers fabricated by thermal diffusion of dopants such as $GeO_{2}$ in hybrid fiber components has an advantage of eliminating lenses for collimation and focusing. An electric furnace is fabricated to heat the fibers locally for the core expansion. We observed an expansion of the mode size at $1.3\mu\textrm{m}$ wavelength by 27% after treating a section of single mode optical fiber at $1250^{\circ}C$ for 10 hours. hours.

• The Journal of Korean Institute of Electromagnetic Engineering and Science
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• v.8 no.1
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• pp.1-12
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• 1997

The acousto-optical spectrometer as a new type backend of the receiver system for radio astronomical observations is manufactured for radio signal analysis. We studied on the effect of Acousto-Optic and Acousto-Optic devices and designed the optics system. We manufactured the optical mount and the CCD detector for deflected beam and interface card. This acousto-optical spectrometer consisted of a laser, optics, acousto-optic deflector, CCD detector and Interface card. This system use He-Ne laser as a light source and use optics to get parallel beam and to focus the deflected beam. Acousto-optic deflector converts IF signal to ultrasonic wave and deflect the laser beam according to the Bragg deflection. The ultra wide band acousto-optic deflector has 1 GHz bandwidth and a total of 2,048 channel Charge Coupled Device for signal detection. In this study, we discuss the theoretical description on the effect of Acousto-optics, the design of the optics, manufacture of optical mount, CCD detector, interface card and we presented the results of experiment. As a result of measurement, we have 1,000 channels bandwidth from CCD channels.