• 한국광학회:학술대회논문집
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• 한국광학회 2009년도 창립 20주년기념 특별학술발표회
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• pp.209-210
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• 2009

• 한국자기학회:학술대회 개요집
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• 한국자기학회 1995년도 추계연구발표회 논문개요집
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• pp.38-39
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• 1995

• 한국광학회:학술대회논문집
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• 한국광학회 2001년도 하계학술발표회
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• pp.26-27
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• 2001

• 한국광학회:학술대회논문집
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• 한국광학회 1999년도 제16회 광학 및 양자전자 학술발표회Proceedings of 16th Optics and Quantum Electronics Conference, 1999
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• pp.64-65
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• 1999

• 한국광학회지
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• 제6권4호
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• pp.259-265
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• 1995

국내 민수용으로 유통되고 있는 20여종의 무반사 안경렌즈들을 선정하여 광학적 특성을 분석하였다. 분광광도계를 사용하여 측정한 반사특성과 투과특성을 렌즈의 굴절력, 각 무반사층들 및 렌즈기층에 의한 영향과 연결시켜 분석하였다. 흡수단 근방에서의 겉보기 흡수스펙트럼은 기층물질에 따라 결정되며 400-700nm의 파장대역에서 대부분의 시료들의 겉보기 흡수스펙트럼과 반사스펙트럼은 강한 양의 상관관계를 보여준다. 예외적으로 기층에 의한 흡수가 큰 렌즈들은 상관관계가 약해지며 이와 같은 기층에 의한 흡수는 무반사 특성에 부정적인 효과를 가진다. 또한 국내에서 제작되는 $SiO_2/TiO_2/SiO_2/ZrO_2/Cr$ 다층박막층을 c-Si 기층위에 성장시키면서 각 단계별로 ex-situ 분광타원해석법으로 분석하여 $TiO_2$ 박막과 $ZrO_2$ 박막의 조밀도가 80% 정도에 불과하며 박막이 두꺼원 짐에 따라 박막에 수직한 방향으로 균일하지 않음을 확인하였다. 마지막으로 실시간, in-suti 측정을 바탕으로하여 엄밀한 사양이 요구되는 다층박막, 초격자박막 등을 재현성있게 성장시킬 수 있는 가능성에 대해 토의하였다.

• 한국진공학회:학술대회논문집
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• 한국진공학회 2012년도 제43회 하계 정기 학술대회 초록집
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• pp.141-141
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• 2012

The electronic and optical properties of Indium Zinc Tin Oxide (IZTO) thin films using gas environment were investigated by X-ray photoelectron spectroscopy (XPS) and reflection electron energy loss spectroscopy (REELS). REELS spectra revealed that the band gaps of IZTO thin films are 3.26, 3.07, and 3.46 eV for water mixed with oxygen, argon mixed with oxygen, and air environments, respectively. The measured band gaps by REELS are consistent with the optical band gaps obtained by UV-Spectrometer. The optical properties represented by the dielectric function $\mathfrak{m}$, the refractive index n, the extinction coefficient k, and the transmission coefficient T of the IZTO thin films with different gas environments were determined from a quantitative analysis of REELS spectra. The calculated transmission from quantitative analysis of REELS spectra shows good agreement with transmission measured by UV-spectrometer. The transmission values of 89% and low electrical resistivity of $3.55{\times}10^{-3}{\Omega}{\cdot}cm$ have been achieved for argon mixed with oxygen which indicates that the gas enviroment plays an important role in improving the electronic and optical properties of films.

• 천문학회보
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• 제36권1호
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• pp.27.2-27.2
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• 2011

The Kepler(NASA) and CoRoT(ESA) space telescopes are surveying thousands of exoplanet for finding Earth-like exoplanets with similar environments of the Earth. Then the TPF(NASA), DARWIN(ESA) and many large-aperture ground telescopes have plan for spectroscopic observations of these earth-like exoplanets in next decades. Now, it has been started to simulate the disk averaged spectra of the earthlike exoplanets for comparing the observed spectra and suggesting solutions of environment of these planets. Previous research, the simulations are based on radiative transfer method, but these are limited by optical models of Earth system and instruments. We introduce a new simulation method, IRT(Integrated Ray Tracing) to overcome limitations of previous method. The 3 components are defined in IRT; 1)Sun model, 2)Earth system model (Atmosphere, Land and Ocean), 3)Instrument model. The ray tracing in IRT is simulated in composed 3D real scale space from inside the sun model to the detector of instrument. The Sun model has hemisphere structure with Lambertian scattering optical model. Atmosphere is composed of 16 distributed structures and each optical model includes BSDF with using 6SV radiative transfer code. Coastline and 5 kinds of vegetation distribution data are used to land model structure, and its non-Lambertian scattering optical model is defined with the semi-empirical "parametric kernel method" used for MODIS(NASA) and POLDER(CNES) missions. The ocean model includes sea ice cap structure with the monthly sea ice area variation, and sea water optical model which is considering non-lambertian sun-glint scattering. Computation of spectral imaging and radiative transfer performance of Earth system model is tested with hypothetical space instrument in IRT model. Then we calculated the disk averaged spectra of the Earth system model in IRT computation model for 8 cases; 4 viewing orientation cases with full illuminated phase, and 4 illuminated phase cases in a viewing orientation. Finally the DAS results are compared with previous researching results of radiative transfer method.

• Applied Science and Convergence Technology
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• 제23권3호
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• pp.113-127
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• 2014

For more than five decades, silicon has dominated the semiconductor industry that supports memory devices, ICs, photovoltaic devices, etc. Photoluminescence (PL) is an attractive silicon characterization technique because it is contactless and provides information on bulk impurities, defects, surface states, optical properties, and doping concentration. It can provide high resolution spectra, generally with the sample at low temperature and room-temperature spectra. The photoluminescence properties of silicon at low temperature are reviewed and discussed in this study. In this paper, silicon bulk PL spectra are shown in multiple peak positions at low temperature. They correspond with various impurities such as In, Al, and Be, phonon interactions, for example, acoustical phonons and optical phonons, different exciton binding energies for boron and phosphorus, dislocation related PL emission peak lines, and oxygen related thermal donor PL emissions.

• 천문학회보
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• 제37권2호
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• pp.108.1-108.1
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• 2012

Previously we introduced ray-tracing based 3D optical earth system model for specular and scattering properties of all components of the system (i.e. clear-sky atmosphere, land surfaces and an ocean surface). In this study, we enhanced 3-dimensional atmospheric structure with vertical atmospheric profiles for multiple layer and cloud layers using Lambertian and Mie theory. Then the phase dependent disk averaged spectra are calculated. The main results, simulated phase dependent disk averaged spectra and light curves, are compared with the 7 bands(300~1000nm) light curves data of the Earth obtained from High Resolution Instrument(HRI) in Deep Impact spacecraft during Earth flyby in 2008. We note that the results are comparable with the observation.

• 한국광학회지
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• 제15권3호
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• pp.193-199
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• 2004

우리는 이중공명 광펌핑(double resonance optical pumping; DROP)효과를 이용하여 루비듐($^{87}$ Rb) 원자의 5P$_{3}$2/-4D$_{3}$2/와 5P$_{3}$2/-4D$_{5}$ 2/ 전이선에서 DROP 스펙트럼을 관측하고, 1.5 $\mu\textrm{m}$ 레이저의 주파수를 무변조 안정화하였다. 관측한 DROP 스펙트럼은 기존의 광-광이중공명(optical-optical double resonance; OODR) 스펙트럼보다 높은 신호대잡음비를 가지며, 약 10 MHz의 좁은 선폭을 갖고 있다. DROP 스펙트럼의 상대적인 세기는 자발방출에 의한 광펌핑 정도로 설명할 수 있었다. DROP스펙트럼에 안정화된 1.5 $\mu\textrm{m}$ 레이저의 주파수 흔들림은 샘플링 시간 0.1초에서 0.2 MHz로 측정되었고, 상대주파수 흔들림은 평균시간 100초에서 약 1${\times}$$10^{-11}$이었다.