• 한국분말재료학회지
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• 제28권4호
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• pp.325-330
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• 2021

In this study, a ZnS film of 8-mm thickness was prepared on graphite using a hot-wall-type CVD technique. The ZnS thick film was then hot isostatically pressed under different pressures (125-205 MPa) in an argon atmosphere. The effects of pressure were systematically studied in terms of crystallographic orientation, grain size, density, and transmittance during the HIP process. X-ray diffraction pattern analysis revealed that the preferred (111) orientation was well developed after a pressure of 80 MPa was applied during the HIP process. A high transmittance of 61.8% in HIP-ZnS was obtained under the optimal conditions (1010℃, 205 MPa, 6 h) as compared with a range of approximately 10% for the CVD-ZnS thick film under a 550-nm wavelength. In addition, the main cause of the improvement in transmittance was determined to be the disappearance of the scattering factor due to grain growth and the increase in density.

• 한국산업융합학회 논문집
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• 제23권6_2호
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• pp.1025-1032
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• 2020

In this paper, we propose a method to classify road weather conditions into rain, fog, and sun using a SVM (Support Vector Machine) classifier after extracting weather features from images acquired in real time using an optical sensor installed on a roadside post. A multi-dimensional weather feature vector consisting of factors such as image sharpeness, image entropy, Michelson contrast, MSCN (Mean Subtraction and Contrast Normalization), dark channel prior, image colorfulness, and local binary pattern as global features of weather-related images was extracted from road images, and then a road weather classifier was created by performing machine learning on 700 sun images, 2,000 rain images, and 1,000 fog images. Finally, the classification performance was tested for 140 sun images, 510 rain images, and 240 fog images. Overall classification performance is assessed to be applicable in real road services and can be enhanced further with optimization along with year-round data collection and training.

• 천문학논총
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• 제37권2호
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• pp.13-31
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• 2022

We observed the symbiotic star AG Dra for a total of 61 nights between April 2004 and December 2021 using the 1.8-m telescope and the high-resolution Echelle spectrograph BOES at the Bohyunsan Optical Astronomy Observatory and obtained 355 frames of spectroscopic data to investigate the variations in its spectral lines. Overnight short-term and long-term changes in prominent emission lines are examined. No short-term changes are found in the line profiles. However, the peak intensity of the Hα emission line exhibits very small variation. In the long-term period, many emission lines including He I λ5875, λ6678, λ7065 and Fe II λ5018 are found to vary reflecting the symbiotic outburst activities. It is noted that He II λ4686 and Raman-scattered O VI λ6830, λ7088 are exceptions, where no significant variations are discernible. One of the noticeable lines is the λ5018 line. Its appearance and disappearance pattern are different from other emission lines, and the line is found to appear in outburst states. The Hα and Hβ lines remain very similar in our spectroscopic monitoring campaign.

• International Journal of Advanced Culture Technology
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• 제10권4호
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• pp.460-469
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• 2022

Increasing interest in the metaverse world these days, interest in realistic content such as 3D displays is growing. In particular, hologram images seen in movies provide viewers with an immersive display that cannot be seen in conventional 2D images. Since the first discovery of holography by Dennis Gabor in 1948, this technology has developed rapidly. Spatially, this beginning of technology like Optical hologram called analog hologram and Digital hologram such as computer-generated hologram (CGH). In analog and digital holograms, a recording angle and a recording wavelength are having important role when reproducing and display hologram. In the hologram, diffraction of light causes by unexpected formed by the synthesis from interference with object and reference light. When recording, the incident light information and mismatched reproduction light reconstruct the hologram in an undesirable direction. Reproduction light that is out of sync with incident light information with initial condition of recording will cause reconstructed image in an undesirable direction. Therefore, we analyze the holographic interference pattern generated by hologram recording in volume holograms using photopolymer and analyze the characteristics that vary depending on the angle of the reproduced light. This is expected to be used as a basic research on various holographic application that may cause as holograms are applied to industries in the future.

• 천문학회보
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• 제46권2호
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• pp.36.1-37
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• 2021

Six images of IRC+10216 taken by the Hubble Space Telescope at three epochs in 2001, 2011, and 2016 are compared in the rest frame of the central carbon star. An accurate astrometry has been achieved with the help of Gaia Data Release 2. The positions of the carbon star in the individual epochs are determined using its known proper motion, defining the rest frame of the star. In 2016, a local brightness peak with compact and red nature is detected at the stellar position. A comparison of the color maps between 2016 and 2011 epochs reveals that the reddest spot moved along with the star, suggesting a possibility of its being the dusty material surrounding the carbon star. Relatively red, ambient region is distributed in an Ω shape and well corresponds to the dusty disk previously suggested based on near-infrared polarization observations. In a larger scale, differential proper motion of multiple ring-like pattern in the rest frame of the star is used to derive the average expansion velocity of transverse wind components, resulting in ~12.5 km s-1 (d/123 pc), where d is the distance to IRC+10216. Three dimensional geometry is implied from its comparison with the line-of-sight wind velocity determined from half-widths of submillimeter emission line profiles of abundant molecules. Uneven temporal variations in brightness for different searchlight beams and anisotropic distribution of extended halo are revisited in the context of the stellar light illumination through a porous envelope with postulated longer-term variations for a period of 10 years.

• 열처리공학회지
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• 제36권4호
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• pp.193-197
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• 2023

Transparent and conducting titanium (Ti) doped indium oxide (TIO) thin films were deposited on the poly-imide (PI) substrate with radio frequency magnetron sputtering and then electron irradiation was conducted on the TIO film's surface to investigate the effect electron irradiation on the crystallization and opto-electrical properties of the films. All x-ray diffraction (XRD) pattern showed two diffraction peaks of the In₂O₂ (431) and (444) planes with regardless of the electron beam irradiation energy. In the AFM analysis, the surface roughness of as deposited films was 3.29 nm, while the films electron irradiated at 700 eV, show a lower RMS roughness of 2.62 nm. In this study, the FOM of as deposited TIO films is 6.82 × 10^-3 Ω^-1, while the films electron irradiated at 500 eV show the higher FOM value of 1.0 × 10^-2 Ω^-1. Thus, it is concluded that the post-deposition electron beam irradiation at 500 eV is the one of effective methods of crystallization and enhancement of opto-electrical performance of TIO thin film deposited on the PI substrate.

• Current Optics and Photonics
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• 제7권4호
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• pp.408-418
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• 2023

Due to the technological limitations of infrared thermography, infrared focal plane array (IFPA) imaging exhibits stripe non-uniformity, which is typically fixed pattern noise that changes over time and temperature on top of existing non-uniformities. This paper proposes a stripe non-uniformity correction algorithm based on scene-adaptive nonlinear filtering. The algorithm first uses a nonlinear filter to remove single-column non-uniformities and calculates the actual residual with respect to the original image. Then, the current residual is obtained by using the predicted residual from the previous frame and the actual residual. Finally, we adaptively calculate the gain and bias coefficients according to global motion parameters to reduce artifacts. Experimental results show that the proposed algorithm protects image edges to a certain extent, converges fast, has high quality, and effectively removes column stripes and non-uniform random noise compared to other adaptive correction algorithms.

• 대한전자공학회논문지SP
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• 제43권2호
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• pp.30-39
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• 2006

홍채 인식은 흥채 근육의 무의 패턴을 이용하여 동일인 여부를 판별하는 연구 분야이다. 이러한 홍채 인식에서 홍채 영상의 품질은 홍채 인식의 성능에 많은 영향을 준다. 이는 흥채 영상이 흐려지면, 홍채 패턴이 변형되어지므로, FRR(False Rejection Error)이 증가되기 때문이다. 홍채 영상을 흐려지게 만드는 주된 요인 가운데 하나가 카메라 렌즈의 초점(focus)이다. 기존의 흥채 인식 카메라는 고정 초점(fixed focusing) 방식과 가변 초점(auto-focusing) 방식이 있다. 고정 초점 방식은 초점 렌즈가 고정되어 있기 때문에 사용자가 직접 자신의 눈을 DOF(Depth of Field) 영역 안에 위치시켜야하고, DOF 영역이 매우 작은 한계가 있다. 가변 초점 방식은 사용자와 카메라 사이의 거리를 측정하여 초점이 잘 맞는 위치로 초점렌즈를 움직여서 선명한 영상을 취득한다. 하지만 부가적인 하드웨어 장비가 필요하기 때문에 카메라의 부피가 늘어나고 비용도 증가되므로 개인 인증을 위해 홍채인식을 하는 핸드폰과 같은 모바일 장비에서 사용되는데 어려움이 따른다. 따라서 본 논문은 이러한 기존의 홍채인식 카메라의 문제점들을 극복하기 위해 부가적인 하드웨어 장비 없이 고정 초점 방식 카메라에서 취득한 홍채 영상을 복원함으로써 소프트웨어적으로 DOF영역을 증가시키는 방법을 제안한다. 기존의 영상 복원 알고리즘은 반복적(iterative) 방법에 의해 최상의 복원 계수(parameter)를 검출하여 영상을 복원하였으나, 본 논문은 초점값을 이용하여 영상의 흐려짐의 정도를 판단하고, 흐려짐의 정도에 따라 미리 정의한 복원 계수를 선택함으로써 빠른 시간 안에 홍채 영상을 복원하는 방법을 제안한다. 실험 결과, Panasonic에서 만든 BM-ET100 카메라의 작동범위(Operation Range)를 48-53cm에서 46-56cm로 증가시킬 수 있었다.

• 한국가금학회지
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• 제18권3호
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• pp.183-196
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• 1991

세계적으로 가장 출현빈도가 높은 혈청형인 마사추셋형 IBV를 발육란에서 증식시킨 다음 요막강액을 채취, 바이러스를 농축 정제하여 항원으로 사용하고 야외 IBV감염계군에서 채취한 혈청중 HI반응에 의해 양성 및 음성혈청을 선발, 표준혈청으로 사용하여 ELISA를 시도한 결과 다음과 같은 성적을 얻었다. 1. 정제항원은 ELISA plate의 well당 40ng 단백량으로 coating하였을 때 높은 P/N치를 나타냈고 혈구응집항원은 well당 1.2~2.5 HA unit로 coating하였을 때 정제항원과 유사한 결과를 보였다. 2. 항원의 coating시 온도와 시간은 37$^{\circ}C$, 1시간이나 4$^{\circ}C$에 12~16시간 처리하였을 때 P/N에서 유의성 있는 차이를 보이지 않았으며 항원을 건조시켜 4$^{\circ}C$에 1개월 보관하여도 항원성의 변화를 인정할 수 없었다. 3 제품이 다른 3종류의 plate에서 항원 coating의 차이를 비교한 결과 제품간에 항원 coating의 균일도와 농도에 있어서 뚜렷한 차이가 인정되었다. 4. 음성혈청희석배수 1：50에서도 비특이 반응은 인정되지 않았으며 가경혈청은 1：100희석했을 때 높은 P/N치를 보여서 screen용 희석배수로 적당하였다. 5. Substrate처리한 후 발색 정도는 15분 이후에는 일정하여 30분까지 변화가 없었으며 이때 발색정지제를 처리하였을 때 치리직후부터 4시간까지도 흡광도에 있어서 유의성 있는 차이가 인정되지 않았다. 6. 74개의 혈청에 대해 ELISA에 의한 P/N치와 HI항체가와의 상관관계는 r＝0.42였으며 HI가 2$^{6}$이상, P/N치 1.4이상을 기준으로 하였을 때 양성 case의 일치율은 98.7%였다. 1. 백신접종 시험계군에서 ELISA와 HI test에 의한 항체 소장 비교에서는 10주째를 제외하고는 양 test에서 유사한 추이를 보였다.

• Bulletin of the Korean Chemical Society
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• 제24권4호
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• pp.446-452
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• 2003

Some new nanohybrid materials have been synthesized by intercalating the oxotitanium(IV) meso-tetrakis(4- sulfonatophenyl) porphyrin$(O=Ti^{(IV)} TSPP)$ into the Zn/Al layered double hydroxides (LDHs), and their structures and photophysical properties have been investigated by various laser spectroscopic techniques. According to the XRD pattern of the synthesized nanohybrid materials, the macrocycle plane of $O=Ti^{(IV)}$ TSPP are grafted perpendicular to the LDH layers. The $O=Ti^{(IV)}$ TSPP-intercalated LDH exhibits band broadening of the absorption spectrum and a blue shift of Q-band as compared to that observed in solution. Resonance Raman spectral measurements demonstrate that the positively charged LDHs give rise to a slight decrease of the electronic density of the porphyrin ring accompanying a small change of the electronic distribution of the $O=Ti^{(IV)}$ TSPP. Consequently the LDH environment affects the energies of the two highest occupied molecular orbitals (HOMOs) of the $O=Ti^{(IV)}$) TSPP, $a_{1u}$ and $a_{2u}$, producing a mixed orbital character. Being consistent with these electronic structural changes of $O=Ti^{(IV)}$ TSPP in LDH, both the fluorescence spectral change and the fsdiffuse reflectance transient measurements imply that the photoexcitation of the $O=Ti^{(IV)}$ TSPP intercalated into LDH undergoes fast relaxation to the O=Ti(IV) $TSPP^+-LDH^- $charge transfer (CT) state within a few picoseconds, followed by a photoinduced electron transfer between the O=Ti(IV) TSPP and LDHs with a rate constant greater than %1×10^{10}S^{-1}$. No evidence is found for back electron transfer. In conclusion, the $O=Ti^{(IV)}$ TSPP intercalated LDH seems to be a possible candidate for an artificial reaction center for an efficient solar energy conversion system.