• 한국광학회:학술대회논문집
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• 한국광학회 1991년도 제6회 파동 및 레이저 학술발표회 Prodeedings of 6th Conference on Waves and Lasers
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• pp.90-93
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• 1991

일곤 레이저의 두 파장(488 nm, 514.5 nm)을 사용하여 은 박막과 은 박막 위에 덧증착한 ZnS 박막의 유일한 광학 상수와 두께를 Kretschmann 구조의 표면 플라즈몬 공명을 이용하여 결정하였다.

• 한국소음진동공학회:학술대회논문집
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• 한국소음진동공학회 2004년도 추계학술대회논문집
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• pp.227-231
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• 2004

Technological advance in information technology has sparked the necessity of small form factor (SFF) optical disk for mobile devices. Small form factor optical disk is highly anticipated to be a next generation storage device because it can be used for a cost-effective way compared with solid state memory. For the application to the 5 mm height small-form-factor optical disk drive, we have presented an optical flying head and swing arm actuator. In this study, we propose a small 1-axis actuator for compensating ficus error and SA due to the variation of cover-layer thickness in the cover-layered small optical disk. The main design issues of the 1-axis actuator are the realization of compact structure and the new support structure of the actuator: Finally, the compensating principle and performance of the 1-axis actuator will be explained.

• 한국광학회지
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• 제30권1호
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• pp.15-22
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• 2019

소산파 기반 집적광학 바이오센서에 적합한 $Si_3N_4$ 립-광도파로 구조에 대한 해석적 분석을 통해서 단일모드 도파조건을 도출하였다. 두-모드 간섭현상을 이용하는 집적광학 바이오센서 구조를 제시하고, 단일모드와 두-모드(감지영역)에 해당되는 립-광도파로 제원인 폭, 립 및 코어 두께 각각에 대해서 $3{\mu}m$, 2 nm, 150 nm와 $3{\mu}m$, 20 nm, 340 nm를 제안하였으며, FMM 전산해석을 통해서 감지영역의 두-모드들에 대한 광학적 특성들을 검토하였다.

• 한국재료학회지
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• 제23권8호
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• pp.469-475
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• 2013

Al-doped ZnO(AZO) thin films were synthesized using atomid layer deposition(ALD), which acurately controlled the uniform film thickness of the AZO thin films. To investigate the electrical and optical properites of the AZO thin films, AZO films using ALD was controlled to be three different thicknesses (50 nm, 100 nm, and 150 nm). The structural, chemical, electrical, and optical properties of the AZO thin films were analyzed by X-ray diffraction, X-ray photoelectron spectroscopy, field-emssion scanning electron microscopy, atomic force microscopy, Hall measurement system, and UV-Vis spectrophotometry. As the thickness of the AZO thin films increased, the crystallinity of the AZO thin films gradually increased, and the surface morphology of the AZO thin films were transformed from a porous structure to a dense structure. The average surface roughnesses of the samples using atomic force microscopy were ~3.01 nm, ~2.89 nm, and ~2.44 nm, respectively. As the thickness of the AZO filmsincreased, the surface roughness decreased gradually. These results affect the electrical and optical properties of AZO thin films. Therefore, the thickest AZO thin films with 150 nm exhibited excellent resistivity (${\sim}7.00{\times}10^{-4}{\Omega}{\cdot}cm$), high transmittance (~83.2 %), and the best FOM ($5.71{\times}10^{-3}{\Omega}^{-1}$). AZO thin films fabricated using ALD may be used as a promising cadidate of TCO materials for optoelectronic applications.

• 한국광학회지
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• 제27권4호
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• pp.143-150
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• 2016

분광광도계로 측정된 반사율 데이터를 활용하여 다층박막 각 층의 두께를 푸리에 변환 방법으로 결정하였다. 이를 위하여 이론적인 3층 다층박막 반사율 데이터를 생성하고 자체 작성한 Matlab 프로그램으로 델타함수의 피크 발생위치로부터 각 층의 두께를 결정하였으며, 박막의 광학적 두께가 730 nm 이상이 되는 경우 결정된 두께 오차는 1.0% 이하임을 알 수 있었다. 이 방법을 사용하여 바 코팅 방법으로 제작된 PI-(얇은 $SiO_2$)-PI 다층박막의 두께를 결정하고 그 결과를 SEM 측정결과와 비교하였다. 본 두께측정 방법은 각 층의 굴절률과 박막의 순서를 미리 인지하고 있어야 하는 단점이 있으나, 비파괴적인 방법으로 빠르게 다층 박막의 두께 분포를 결정할 수 있는 방법임을 확인하였다.

• Journal of the Optical Society of Korea
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• 제12권2호
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• pp.112-117
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• 2008

Single-mode propagation conditions of X-ray waveguides are investigated by numerical calculations in order to understand the importance of waveguide design parameters, such as core thickness and the optical constants of waveguide materials, on the transmission and coherence properties of the waveguide. The simulation code for mode analyzing is developed based on a numerical solution of the parabolic wave equation. The initial boundary value problem is solved numerically using a finite-difference scheme based on the Crank-Nicolson scheme. The E-field intensities in a core layer are calculated at an X-ray energy of 8.0 keV for air and beryllium(Be) core waveguides with different cladding layers such as Pt, Au, W, Ni and Si to determine the dependence on waveguide materials. The highest E-field intensity radiated at the exit of the waveguide is obtained from the Pt cladded beryllium core with a thickness of 20 nm. However, the intensity from the air core waveguide with Pt cladding reaches 64% of the Be-Pt waveguide. The dependence on the core thickness, which is the major parameter used to generate a single mode in the waveguide, is investigated for the air-Pt, and Be-Pt waveguides at an X-ray energy of 8.0 keV. The mode profiles at the exit are shown for the single mode at a thickness of up to 20 nm for the air-Pt and the Be-Pt waveguides.

• 한국전기전자재료학회논문지
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• 제11권10호
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• pp.903-910
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• 1998

Ti:LiNbO$_3$ optical waveguides have been fabricated by Ti-diffusion in wet oxygen atmosphere. The fabrication conditions of furnace temperature, diffusion time and bubbler temperature were 105$0^{\circ}C$, 8 hours and 9$0^{\circ}C$, respectively and Ti thickness was varied from 700$\AA$ to 1500$\AA$. In this paper, the nearfield patterns, mode sizes (hirizontal/vertical) and insertion loss of waveguides were discussed at wavelength 1550 nm ad function of Ti thickness. With the planar waveguide, the effective index change and diffusion depth were calculated at 632.8nm using the prism coupling method. From these results, the best Ti thickness in our conditions seems like to by 1200$\AA$~1300$\AA$.

• 한국광학회지
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• 제12권6호
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• pp.472-478
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• 2001

가변입사각 분광타원법(Variable Angle Spectroscopic Ellipsometry)을 사용하여 유기발광소자(OLED)의 발광층인 유기박막 의 광학상수와 두께를 결정하였다. 광투과영역에서 모델링분석으로 박막의 평균두께와 굴절률 분산식을 결정하고, 광흡수영역으로 확장하여 유기막의 다층구조, 각 층의 두께와 밀도 그리고 각 파장에서의 복소굴절률을 결정하였다. 분광광도계를 사용하여 구한 투과율 스펙트럼을 가변입사각 분광타원법을 사용하여 결정한 다층구조 및 복소굴절률로 계산한 투과율 스펙트럼과 비교하여 분석의 정확성을 확인하였다.

• 대기
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• 제25권3호
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• pp.521-528
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• 2015

In this study star photometry was applied to retrieve aerosol optical thickness (AOT) at night. The star photometry system consisted of small refractor, optical filters, CCD camera, and driving mount and was located in Suwon. The calibration constants were retrieved from the astronomical Langley method but standard deviations of these were more than 10% of the mean values. After the calibration the nighttime AOT was retrieved and cloud-screened in clear six days from 25 Nov. 2014 to 17 Jan. 2015. To estimate the quality of the measurements the nighttime AOT was combined with daytime AOT retrieved from sky-radiometer that was located in Seoul and 17 km away from the star photometry system. In spite of the uncertainty of the calibration constants and the spatial difference of two observation systems, the temporal changes of the nighttime AOT coincided with the daytime. The nighttime ${\AA}ngstr{\ddot{o}}m$ exponent was about 20% lower and more variable than the daytime because of the uncertainty of the calibration constants. If the calibration process is more precise, the combination of star and sun or sky photometry system can monitor the air pollution day and night constantly.

• 한국광학회지
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• 제6권3호
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• pp.245-256
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• 1995

Fourier 면환을 이용하여 불균일 굴절률 박막의 rugate 필터를 설계하였으며 rugate 필터의 반사율, 대역폭, 광학 두께, Q 함수 등을 변화시키며 Fourier 변환의 여러 가지 특성을 조사하였다. 주어진 단선 및 이중 rugate 필터의 과녁 스펙트럼에 불균일 굴절률 박막의 스펙트럼을 맞추기 위하여 merit 함수를 사용하였으며 merit 값이 최소가 되도록 Q 함수를 반복계산하여 수정하였다. Sossi, Bovard, Fabricius가 각각 유도한 세 종류의 Q함수를 반복계산 횟수, merit 함수의 값, 최적 광학두께 등의 관점에서 비교하였다. 반사율이 높은 rugate 필터 설계에는 반복계산 수정 후 반사율이 과녁스펙트럼에 가까운 Bovard와 Fabricius의 Q함수가 적당하며, 광학 두께는 최소 광학두께만 넘으면 반복계산 수정과정을 이용하여 과녁반사율을 맞출 수 있으므로 반사대역폭이 허용하는 광학두께로 결정하면 될 것이다.