• 한국재료학회지
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• 제20권4호
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• pp.194-198
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• 2010

Cubic boron nitride (c-BN) is a promising material for use in many potential applications because of its outstanding physical properties such as high thermal stability, high abrasive wear resistance, and super hardness. Even though 316L austenitic stainless steel (STS) has poor wear resistance causing it to be toxic in the body due to wear and material chips, 316L STS has been used for implant biomaterials in orthopedics due to its good corrosion resistance and mechanical properties. Therefore, in the present study, c-BN films with a $B_4C$ layer were applied to a 316L STS specimen in order to improve its wear resistance. The deposition of the c-BN films was performed using an r.f. (13.56 MHz) magnetron sputtering system with a $B_4C$ target. The coating layers were characterized using XPS and SEM, and the mechanical properties were investigated using a nanoindenter. The friction coefficient of the c-BN coated 316L STS steel was obtained using a pin-on-disk according to the ASTM G163-99. The thickness of the obtained c-BN and $B_4C$ were about 220 nm and 630 nm, respectively. The high resolution XPS spectra analysis of B1s and N1s revealed that the c-BN film was mainly composed of $sp^3$ BN bonds. The hardness and elastic modulus of the c-BN measured by the nanoindenter were 46.8 GPa and 345.7 GPa, respectively. The friction coefficient of the c-BN coated 316L STS was decreased from 3.5 to 1.6. The wear property of the c-BN coated 316L STS was enhanced by a factor of two.

• 한국정보디스플레이학회:학술대회논문집
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• 한국정보디스플레이학회 2003년도 International Meeting on Information Display
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• pp.7-10
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• 2003

Samsung SDI has developed a full color 5.0" WVGA AMOLED display with top emission and a super fine pitch of 0.1365mm(l86ppi), the world's highest resolution OLED display ever reported to date. Scan driver circuits and demux circuit were integrated into the display panel, using low temperature poly-Si TFT CMOS technology, and data driver circuit were mounted using COG chips. Peak luminescence was greater than 300cd/ $m^2$ with power consumption of 500mW with 30% of the pixels on illuminated.

• 한국통신학회논문지
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• 제35권9C호
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• pp.778-785
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• 2010

본 논문에서는 IR-UWB 시스템에서의 채널추정 및 다중경로 지연시간 분석을 통한 고 정밀 거리추정 기법을 제안하고자 한다. IR-UWB 무선 신호를 송수신 할 때 정밀한 거리 추정을 위하여 무선채널을 경유한 신호의 전파 도달 시간을 측정하는 Time of Arrival 추정 기법에 의한 고 정밀 거리추정 방식을 수행 하였다. 제안된 기법에서는 Minimum Mean Square Error 또는 Zero Forcing 등의 채널추정 기법과 지연시간 추정 기법인 Matrix Pencil (MP) 기법을 합하여 송수신기 간의 존재하는 다중경로 중에 IR-UWB 펄스보다 더 좁은 간격으로 중첩 수신된 다중경로를 분석하여 수 cm이내의 정밀한 거리를 추정할 수 있음을 보였다. 또한, 제안된 기법을 적용한 시스템의 거리 추정 성능을 IEEE 802.15.4a 채널 모델 별로 비교 분석하였으며, MP parameter 값의 변화에 따른 거리 추정 성능과 연산량 변화를 컴퓨터 시뮬레이션을 통해 분석 하였다.

• 대한전자공학회논문지
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• 제27권2호
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• pp.16-30
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• 1990

지금까지 마이크로웨이브 영상은 주로 파수영역의 해석에 의해 2차원 푸리에 역변환으로 물체의 영상을 재현하였다. 본 논문에서는 공간영역에서 코히어런트 단층촬영 방법으로 영상을 제한할 수 있는 새로운 식을 유도하고 X-ray 단층촬영에 널리 이용되고 있는 filtered-backprojection 알고리듬을 적용하여 line 및 원통 도체에 대한 영상을 수치계산에 의해 재현하였다. 제시된 공간영역의 해석은 기존의 파수영역의 문제점인 interpolation 및 원점에 대칭인 도체의 영상재현시 나타나는 영상의 artifact을 완전히 해결할 수 있음은 물론, 보다 좋은 영상의 질을 얻을 수 있었다. 또한 파수영역의 해석과는 달리, 모멘트 방법을 적용하여 좁은 주파수 대역폭으로도 초고해상도를 얻을 수 있는 가능성을 line 물체의 영상을 통해 보였다.

• 디지털융복합연구
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• 제12권11호
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• pp.233-239
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• 2014

초고해상도 콘텐츠는 파일 크기가 매우 크기 때문에 기존의 부호화 기술로는 네트워크를 통해 전송하는 것이 불가능하다. 고효율의 부호화 기법인 HEVC를 이용하면 네트워크 전송이 가능하나 압축시간이 많이 필요하기 때문에 분산 트랜스코딩 시스템이 필요하다. 분산 트랜스코딩 시스템은 데이터를 분산하여 저장한 뒤 다수의 노드를 이용하여 부호화한다. 그러나 분산 트랜스코딩 시스템은 분산된 정보가 노출되거나 내부관리자의 공격에 취약하다는 문제점이 있다. 본 논문에서는 초고해상도 콘텐츠를 트랜스코딩 할 때, 분산 트랜스코딩 시스템의 기밀성이 보장되지 않는다는 문제점을 해결하고자 한다. 우리는 SNA를 이용하여 데이터 노드에서 HEVC로 부호화된 콘텐츠 데이터를 비밀분산기법을 통해 암호화하여 저장했다. 결과적으로 안전한 분산 트랜스코딩이 가능하고, 내부관리자의 공격을 방지할 수 있다.

• 천문학회지
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• 제32권1호
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• pp.41-53
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• 1999

We have carried out high-resolution observations along one-dimensional cuts through the three Galactic super-shells GS 064-01-97, GS 090-28-17, and GS 174+02-64 in the HI 21 cm and CO J=l-0 lines. By comparing the HI data with IRAS data, we have derived the distributions of the $I_{100}$ and $T_{100}$ excesses, which are, respectively, the 100 ${\mu}m$ intensity and 100 ${\mu}m$ optical depth in excess of what would be expected from HI emission. We have found that both the $I_{100}$ and $T_{100}$ excesses have good correlations with the CO integrated intensity W co in all three supershells. But the $I_{100}$ excess appears to underestimate $H_2$ column density N($H_2$) by factors of 1.5-3.8. This factor is the ratio of atomic to molecular infrared emissivities, and we show that it can be roughly determined from the HI and IRAS data. By comparing the $T_{100}$ excess with $W_{co}$, we derive the conversion factor X $\equiv$ N ($H_2$) /$W_{co}{\simeq}$ 0.26 - 0.66 in the three supershells. In GS 090- 28-17, which is a very diffuse shell, our result suggests that the region with N($H_2$) $\le$ $3 {\times} 10^{20} cm^{-2}$ does not have observable CO emission, which appears to be consistent with previous results indicating that diffuse molecular gas is not observable in CO. Our results show that the molecular gas has a 60/100 ${\mu}m$ color temperature $T_d$ lower than the atomic gas. The low value of $T_d$ might be due either to the low equilibrium temperature or to the lower abundance of small grains, or a combination of both.

• 천문학회보
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• 제37권2호
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• pp.142.1-142.1
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• 2012

During the photometric runs of the eclipsing binary V432 Per in 2006, we serendipitously discovered peculiar light variations of GSC 2855-0585 that imaged on the same target field. Its brightness decreased about 0.02 mag for about 0.15 days in all B, V, and R bands. The depth, duration, and box-shaped light curves are very similar to those of typical transiting exoplanets. We gathered the time-series data of GSC 2855-0585 from the SuperWASP public archive and detected the same light variations with a period of about 2.406 days. The period and transitlike features were confirmed by photometric follow-up observations at a predicted epoch in 2010 November. In order to estimate the mass of the companion that produced the light variations, we obtained 10 high-resolution spectra with different orbital phases in 2010 November and 2011 October-December. The radial velocities showed large variations of about 44 km/s. It indicates that the transitlike light variations do not originate from a transiting exoplanet, but from the single-lined spectroscopic eclipsing binary with a cool dwarf companion. Using the photometric and spectroscopic data, we estimated the physical parameters of the eclipsing binary GSC 2855-0585, such as orbital period, effective temperature, surface gravity, and mass.

• 한국수자원학회:학술대회논문집
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• 한국수자원학회 2012년도 학술발표회
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• pp.20-25
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• 2012

New Zealand suffers from regular floods, these being the most common source of insurance claims for damage from natural hazard events in the country. This paper describes the origin and distribution of the largest floods in New Zealand, and describes the systems used to monitor and predict floods. In New Zealand, broad-scale heavy rainfall (and flooding), is the result of warm moist air flowing out from the tropics into the mid-latitudes. There is no monsoon in New Zealand. The terrain has a substantial influence on the distribution of rainfall, with the largest annual totals occurring near the South Island's Southern Alps, the highest mountains in the country. The orographic effect here is extreme, with 3km of elevation gained over a 20km distance from the coast. Across New Zealand, short duration high intensity rainfall from thunderstorms also causes flooding in urban areas and small catchments. Forecasts of severe weather are provided by the New Zealand MetService, a Government owned company. MetService uses global weather models and a number of limited-area weather models to provide warnings and data streams of predicted rainfall to local Councils. Flood monitoring, prediction and warning are carried out by 16 local Councils. All Councils collect their own rainfall and river flow data, and a variety of prediction methods are utilized. These range from experienced staff making intuitive decisions based on previous effects of heavy rain, to hydrological models linked to outputs from MetService weather prediction models. No operational hydrological models are linked to weather radar in New Zealand. Councils provide warnings to Civil Defence Emergency Management, and also directly to farmers and other occupiers of flood prone areas. Warnings are distributed by email, text message and automated voice systems. A nation-wide hydrological model is also operated by NIWA, a Government-owned research institute. It is linked to a single high resolution weather model which runs on a super computer. The NIWA model does not provide public forecasts. The rivers with the greatest flood flows are shown, and these are ranked in terms of peak specific discharge. It can be seen that of the largest floods occur on the West Coast of the South Island, and the greatest flows per unit area are also found in this location.

• Molecules and Cells
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• 제39권7호
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• pp.566-572
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• 2016

Lysosomes are cellular organelles containing diverse classes of catabolic enzymes that are implicated in diverse cellular processes including phagocytosis, autophagy, lipid transport, and aging. Lysosome-associated membrane proteins (LAMP-1 and LAMP-2) are major glycoproteins important for maintaining lysosomal integrity, pH, and catabolism. LAMP-1 and LAMP-2 are constitutively expressed in Salmonella-infected cells and are recruited to Salmonella-containing vacuoles (SCVs) as well as Salmonella- induced filaments (Sifs) that promote the survival and proliferation of the Salmonella. LAMP-3, also known as DC-LAMP/CD208, is a member of the LAMP family of proteins, but its role during Salmonella infection remains unclear. DNA microarray analysis identified LAMP-3 as one of the genes responding to LPS stimulation in THP-1 macrophage cells. Subsequent analyses reveal that LPS and Salmonella induced the expression of LAMP-3 at both the transcriptional and translational levels. Confocal Super resolution N-SIM imaging revealed that LAMP-3, like LAMP-2, shifts its localization from the cell surface to alongside Salmonella. Knockdown of LAMP-3 by specific siRNAs decreased the number of Salmonella recovered from the infected cells. Therefore, we conclude that LAMP-3 is induced by Salmonella infection and recruited to the Salmonella pathogen for intracellular proliferation.

• 방송공학회논문지
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• 제24권3호
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• pp.401-410
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• 2019

본 논문에서는 SHVC 부호화 성능 개선을 위하여 딥러닝 기반 계층간 예측을 위한 참조 픽처 생성 방법을 제안한다. 새로운 참조 픽처를 생성하기 위하여 DCT-IF기반 업샘플링 된 픽처를 VDSR 네트워크를 이용한 필터링을 진행하는 구조와 SHVC 계층간 참조 픽처를 생성하기 위한 트레이닝 방법에 대해 설명한다. 제안하는 방법은 SHM 12.0 기반으로 구현되어 있다. 성능 평가를 위하여 사전 학습을 이용하여 계층간 예측 픽처를 생성하는 방법과 비교를 진행하였다. 그 결과 상위 계층의 부호화 성능은 사전 학습을 이용한 방법 대비 최대 13.14%의 비트 감소, SHM 대비 최대 15.39%의 비트 감소율을 보였고, 평균 6.46%의 비트 감소율을 보였다.