• 제목/요약/키워드: UV reflection

검색결과 131건 처리시간 0.026초

자외선 및 고에너지 가시광 차단 기능을 갖는 눈 건강을 위한 폴리머 안경렌즈 (Polymer Eyeglass Lens with Ultraviolet & High-Energy Visible Light Blocking Function for Eye Health)

  • 김기출
    • 한국산학기술학회논문지
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    • 제21권12호
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    • pp.10-15
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    • 2020
  • 파장 400 nm 이하의 자외선은 눈 건강에 매우 해롭다. 또한 고에너지 가시광도 망막 세포에 영향을 줄 수 있음이 최근에 밝혀졌다. 따라서 자외선 및 고에너지 가시광 차단 기능의 안경렌즈 개발이 시대적으로 요청되고 있다. 본 연구에서는 m-자일릴렌 디이소시아네이트 모노머와 2,3-bis((2-mercaptoethyl)thio)-1-propanethiol 모노머 및 벤트리아졸 UV 흡수제, 알킬인산에스터 이형제, 안료혼합물(CI solvent violet 13), 이염화부틸주석 촉매제 등의 혼합물을 인젝션 몰드 방법으로 열중합 공정을 적용하여, 굴절률 1.67의 고굴절률 폴리머 안경렌즈를 제조하였다. 제조된 폴리머 안경렌즈의 양면에 전자빔 진공증착 시스템으로 다층 반사방지 코팅을 하였다. 제조된 안경렌즈의 자외선 및 고에너지 가시광 차단 기능을 UV-visible spectrophotometer로 분석하였다. 그 결과 UV 흡수제를 0.5wt% 첨가한 폴리머 안경렌즈가 411 nm 파장 이하의 자외선 및 고에너지 가시광을 99 % 이상 차단하였다. 또한 460 ~ 660 nm 파장의 명소시 시각 민감도 10% 이상의 영역에서 평균 투과율이 97.9%를 나타내어 명소시에서 선명한 상을 얻을 수 있었다.

금속불순물 제거를 위한 UV/ozone과 HF 세정연구 (The study on the Removal of Metallic Impurities with using UV/ozone and HF cleaning)

  • 이원준;전형탁
    • 한국재료학회지
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    • 제6권11호
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    • pp.1127-1135
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    • 1996
  • 반도체 소자가 고집적화 됨에 따라 단위공정의 수가 증가하게 되었고 동시에 실리콘 기판의 오염에 대한 문제가 증가하였다. 실리콘 기판의 주 오염물로는 유기물, 파티클, 금속분순물 등이 있으며 특히, Cu와 Fe과 같은 금속불순물은 이온주입 공정, reactive ion etching, photoresist ashing과 같은 실 공정 중에 1011-1013atoms/㎤정도로 오염이 되고 있다. 그러나 금속불순물 중 Cu와 같은 전기음성도가 실리콘 보다 큰 오염물질은 일반적인 습석세정방법으로는 제거하기 힘들다. 따라서 본 연구에서는 Cu와 Fe과 같은 금속불순물을 제거할 목적을 건식과 습식 세정방법을 혼합한 UV/ozone과 HF세정을 제안하여 실시하였다. CuCI2와 FeCI2 표준용액으로 실리콘 기판을 인위적 오염한 후 split 1(HF-only), split 2 (UV/ozone+HF), split 3 (UV/ozone + HF 2번 반복), split 4(UV/ozone-HF 3번 반복)를 실시하였고 TXRF(Total Reflection X-Ray Fluorescence)와 AFM(Atomic Force Microscope)으로 금속불순물 제거량과 표면거칠기를 각각 측정하였다. 또한 contact angle 측정으로 세정에 따른 표면상태도 측정하였다. TXRF 측정결과 split 4가 가장 적은 양의 금속불순물 잔류량을 보였으며 AFM 분석을 통한 표면거칠기도 가장 작은 RMS 값을 나타내었다. Contact angle 측정 결과 UV/ozone 처리는 친수성 표면을 형성하였고 HF처리는 소수성 표면을 형성하였다.

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Spectral-shape-controllable Chirped Fiber Bragg Grating with a Photomechanical Microactuator: Simulation and Experiment

  • Moon, Jong-Ju;Ko, Youngmin;Park, Su-Jeong;Ahn, Tae-Jung
    • Current Optics and Photonics
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    • 제4권6호
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    • pp.477-482
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    • 2020
  • Recently, one of the authors has been reported an optically tunable fiber Bragg grating (FBG) with a photomechanical polymer. It was based on a typical FBG with a downsized diameter of 60 ㎛, coated with azobenzene-containing polymer material. Azobenzene is a well-known reversibly photomechanical stretchable material under ultraviolet (UV) light. The small part of the functional-coating region on the FBG absorbed UV light, which pulled the UV-exposed part of the grating. It was selectable as tunable FBG or tunable chirped FBG, by adjusting the position of UV exposure on the grating. As proof of concept for the tunable FBG device, the characteristics just including UV-induced center-wavelength shift and spectral-width changes of the device were reported. In this paper, we report for the first time that the microactuator makes it possible to control the spectral shape of the FBG reflection, according to the specifications (shape and intensity) of the UV beam that reaches the FBG coated with the azobenzene polymer. In addition, we provide the group-delay profiles for the chirped FBG, so that the sign of its dispersion (normal or anomalous) can be tailored by simply selecting the moving direction of the UV light's displacement in the experiment.

마모 및 나노 압입 시험을 이용한 PUA계 레진의 내구성 비교 (Comparison of Durability for PUA Type Resin using Wear and Nano-indentation Test)

  • 최현민;권신;정윤교;조영태
    • 한국기계가공학회지
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    • 제17권5호
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    • pp.8-15
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    • 2018
  • Films with special properties (e.g., water-repellent films, optical films, anti-reflection films, and flexible films) are referred to as functional films. Recently, there has been interest in fine patterning methods for film fabrication. In particular there have been many studies that use a UV nanoimprint process involving a UV curing method. In this paper, a polymer film was fabricated by the UV nanoimprint process with a micro-pattern, and its durability was evaluated by a wear test and a nano-indentation test. The film mechanical properties (such as coefficient of friction, hardness, and modulus of elasticity) were measured. Moreover, the choice of PUA type resin used in the UV nanoimprint process was confirmed to impact the durability of the thin film. Despite making the polymer film samples using the same method and PUA type resin, different coefficient of friction, hardness, and modulus of elasticity values were obtained. PUA 4 resin had the most favorable coefficient of friction, hardness, and modulus of elasticity. This material is predicted to produce a high durability functional film.

Voxel-wise UV parameterization and view-dependent texture synthesis for immersive rendering of truncated signed distance field scene model

  • Kim, Soowoong;Kang, Jungwon
    • ETRI Journal
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    • 제44권1호
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    • pp.51-61
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    • 2022
  • In this paper, we introduced a novel voxel-wise UV parameterization and view-dependent texture synthesis for the immersive rendering of a truncated signed distance field (TSDF) scene model. The proposed UV parameterization delegates a precomputed UV map to each voxel using the UV map lookup table and consequently, enabling efficient and high-quality texture mapping without a complex process. By leveraging the convenient UV parameterization, our view-dependent texture synthesis method extracts a set of local texture maps for each voxel from the multiview color images and separates them into a single view-independent diffuse map and a set of weight coefficients for an orthogonal specular map basis. Furthermore, the view-dependent specular maps for an arbitrary view are estimated by combining the specular weights of each source view using the location of the arbitrary and source viewpoints to generate the view-dependent textures for arbitrary views. The experimental results demonstrate that the proposed method effectively synthesizes texture for an arbitrary view, thereby enabling the visualization of view-dependent effects, such as specularity and mirror reflection.

근접장 마이크로파 현미경을 이용한 Copper(II)-phthalocyanine 박막의 특성 연구 (Characterization of thin film properties of Copper(II)-Phthalocyanine using a near-field scanning microwave microscope)

  • 박미화;이기진
    • 한국전기전자재료학회:학술대회논문집
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    • 한국전기전자재료학회 2003년도 추계학술대회 논문집 Vol.16
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    • pp.460-463
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    • 2003
  • We report the microwave reflection coefficient $S_{11}$ of copper(II)-phthalocyanine(CuPc) using a near-field microwave microscope(NSMM) in order to understand the intrinsic electromagnetic properties of organic materials. For a NSMM system, a high-quility microstip resonator coupled with a dielectric resonator was used. The reflection coefficient $S_{11}$ was changed by the preparation conditions of CuPc thin films. We compared the reflection coefficient with crystal phase, surface morphology, UV absorption spectra and x-ray diffraction results.

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UV 임프린트 공정을 이용한 평판형 광도파로 기반의 집적형 분광 모듈 제작 (Fabrication of Monolithic Spectrometer Module Based on Planar Optical Waveguide Platform using UV Imprint Lithography)

  • 오승훈;정명영;김환기;최현용
    • 마이크로전자및패키징학회지
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    • 제22권3호
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    • pp.73-77
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    • 2015
  • 본 논문에서는 저가로 쉽게 제작할 수 있는 구조를 지닌 단일칩 형태의 고분자 기반 평판형 분광모듈을 제안하였다. 제안된 분광모듈은 UV 임프린트 기법에 의해 제작되어진 비등간격 나노회절격자와 오목거울이 포함된 평판형 광도파로로 구성되어진다. 회절효율을 향상시키기 위해 나노회절격자의 구조는 $25^{\circ}$의 블레이징 각도와 100nm의 선폭을 가지도록 설계, 제작되었다. 평판형 분광모듈은 700 nm 대역폭과 10 nm 분해능을 가짐을 확인하였다. 이러한 집적형 고분자 분광모듈은 다양한 센서 시스템에 적용될 수 있을 것으로 기대된다.

Radiative Transfer Model of Dust Attenuation Curves in Clumpy, Galactic Environments

  • 선광일
    • 천문학회보
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    • 제41권2호
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    • pp.40.2-40.2
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    • 2016
  • The attenuation of starlight by dust in galactic environments is investigated through models of radiative transfer in a spherical, clumpy interstellar medium (ISM). We show that the attenuation curves are primarily determined by the wavelength dependence of absorption rather than by the underlying extinction (absorption+scattering) curve; the observationally derived attenuation curves cannot constrain a unique extinction curve unless the absorption or scattering efficiency is specified. Attenuation curves consistent with the Calzetti curve are found by assuming the silicate-carbonaceous dust model for the Milky Way (MW), but with the $2175{\AA}$ bump suppressed or absent. The discrepancy between our results and previous work that claimed the Small Magellanic Cloud dust to be the origin of the Calzetti curve is ascribed to the difference in adopted albedos; we use the theoretically calculated albedos whereas the previous ones adopted empirically derived albedos from observations of reflection nebulae. It is found that the model attenuation curves calculated with the MW dust are well represented by a modified Calzetti curve with a varying slope and UV bump strength. The strong correlation between the slope and UV bump strength, as found in star-forming galaxies at 0.5 < z < 2.0, is well reproduced if the abundance of the UV bump carriers is assumed to be 30-40% of that of the MW-dust; radiative transfer effects lead to shallower attenuation curves with weaker UV bumps as the ISM is more clumpy and dustier. We also argue that some of local starburst galaxies have a UV bump in their attenuation curves, albeit very weak.

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실리콘 수지 TIR 선형 렌즈 제작 및 365 nm 파장대역 UV LED 조사기 광원 개발 (Fabrication of Silicone Resin TIR Linear Lens and Development of 365 nm Wavelength UV LED Light Source)

  • 성준호;유순재
    • 한국전기전자재료학회논문지
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    • 제31권6호
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    • pp.433-436
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    • 2018
  • A total internal reflection (TIR) linear lens of size $190(W){\times}5(D){\times}2.1(H)mm^3$ has a directivity of $25^{\circ}$ and was made of a polydimethysiloxane (PDMS) silicone resin with a refractive index of 1.4 and a transmittance of 93% at 365 nm UV wavelength. A light source with a size of $190{\times}25.5mm^2$ was fabricated by installing a TIR linear lens on a chip on board (COB) type LED module mounted with a $1.1{\times}1.1mm^2$ size UV LED. The optical characteristics of the light source showed a maximum irradiation density of $3,840mW/cm^2$ at a working distance of 5 mm and a high uniformity of 91.6% over a $150{\times}25mm^2$ irradiation area. The thermal characteristics of the light source were measured at a supply current of 500 mA. The saturation temperature was reached after 30 min of operation, and measured to be $95^{\circ}C$.