• 한국컴퓨터그래픽스학회논문지
• /
• 제7권3호
• /
• pp.1-7
• /
• 2001

본 논문에서는 canal 곡면의 투시 윤곽곡선 (perspective silhouette)에 대한 매개변수화 (parametrization) 방법과 윤곽곡선을 이루는 모든 연결된 구성요소 (connected component)를 발견하는 효율적이고 안정성 있는 알고리즘을 제시한다. Canal 곡면은 반경이 변화하면서 이동하는 구 (moving sphere)의 외곽곡면 (envelope surface)이며, 구의 중심점의 궤적을 나타내는 곡선 C(t)와 구의 반경 함수 r(t)에 의해 정의된다. 이동 구는 canal 곡면과 원에서 교차한다. Canal 곡면을 원의 집합으로 분할함으로써, 각각의 원 위에서 주어진 관측점에 대한 투시적 윤곽곡선을 구성하는 점을 계산하여 매개변수화하는 방법을 제시한다. 고정된 중심점 $C(t_*)$와 반경 $r(t_*)$를 갖는 이동 구는 canal 곡면과 하나의 원 $K(t_*)$에서 교차한다. 또한 이동 구를 관측점에서 볼 때의 윤곽곡선도 다른 하나의 원 $Q(t_*)$을 구성한다. 두 원 $K(t_*)$와 $Q(t_*)$가 한 점에서 접하게 되는 t의 값을 구함으로써 canal 곡면에 대한 윤곽곡선을 이루는 모든 연결된 구성요소를 발견하는 효율적인 방법을 제시한다.

• Journal of Microbiology and Biotechnology
• /
• 제22권11호
• /
• pp.1580-1587
• /
• 2012

Japanese encephalitis virus (JEV) envelope (E) protein holds great promise for use in the development of a recombinant vaccine. Purified recombinant E (rE) protein may be useful for numerous clinical applications; however, there are limitations in using the Escherichia coli expression system for producing high-quality rE protein. Therefore, in this study, the yeast expression system was used to generate the rE protein. For protein production using the yeast system, the full-length JEV E gene was cloned into Pichia pastoris. SDS-PAGE and immunoblotting analysis demonstrated that the rE protein had a molecular mass of 58 kDa and was glycosylated. The predicted size of the mature unmodified E protein is 53 kDa, suggesting that post-translational modifications resulted in the higher molecular mass. The rE protein was purified to greater than 95% purity using combined ammonium sulfate precipitation and a SP-Sepharose Fast Flow column. This purified rE protein was evaluated for immunogenicity and protective efficacy in mice. The survival rates of mice immunized with the rE protein were significantly increased over that of Hyphantria cunea nuclear polyhedrosis virus E protein (HcE). Our results indicate that the rE protein expressed in the P. pastoris expression system holds great promise for use in the development of a subunit vaccine against JEV.

• 한국수자원학회:학술대회논문집
• /
• 한국수자원학회 1986년도 제28회 수공학연구발표회논문초록집
• /
• pp.93-101
• /
• 1986

본 연구는 하천유역에 있어서, 대규모 수공구조물의 설계홍수량 결정을 위한 최대가능강수량(PMP)분석 및 적용에 그 목적이 있다. PMP는 수문기상학적 방법, 통계학적 방법, 포격선 방법으로 산정하였으며, 최대가능홍수량(PMP)은 합성단위도법과 Chow 방법으로 산정하였다. 각 방법에 의한 PMP를 비교해 본 결과, 통계학적 방법, 수문기상학적 방법, 포격선 방법의 크기 순으로 나타나고 있음을 알 수 있었으며, 산정된 PMP를 기왕의 최대강수량과 비교해 본 결과 수문기상학적 방법이 기상학적 제요소를 고려한 방법이 가장 타당한 방법이라고 사료된다. 산정된 PMP 및 PMF를 확률 수문량과 비교해 본 결과 수문기상학적 방법 및 통계학적 방법은 재현기간 1000년 확률 수문량을 다소 상회하는 것으로 나타났으며, 포격선 방법은 재현기간 200~500년 확률 수문량에 접근하고 있음을 알 수 있었다. 대규모 수공 구조물의 설계에 있어서 위험도를 고려할 경우에는 PMP로부터 PMF를 산정하는 것이 타당할 것이다.

• 한국군사과학기술학회지
• /
• 제20권2호
• /
• pp.255-263
• /
• 2017

An infrared-guided missile has been emerging as a major threat against combat aircraft due to its passive guidance characteristics and with recent advances in stealth technology. Hence, the infrared stealth technology and its effectiveness-evaluation technique become more significant than ever before. In this study, we applied missile aerodynamics to lethal range calculation which allowed more precise prediction. CFD analyses were newly involved in estimating drag force characteristics of an infrared-guided missile. Velocity profiles during flight period of the missile were constructed utilizing these drag characteristics and then incorporated into our in-house code to predict corresponding lethal ranges. The results showed that the present method can predict lethal range more appropriately than the previous one with constant velocity profile. As one of the results, if a fighter gains altitude more which reduces less drag of the attacking missile, then the lethal envelope increases significantly more compared to the lock-on envelope.

• 한국건축시공학회지
• /
• 제16권6호
• /
• pp.579-585
• /
• 2016

3차원 이미지 스캐닝 기술은 복잡한 비정형 건축물의 외피의 정확한 형상과 위치 데이터를 확보하는데 효과적이다. 3차원 이미지 스캐닝 기술의 세부 과정인 점 군집화, 메쉬표면 분리, 넙스 표면 생성, 파라메트릭 솔리드 모델을 통하여 비정형 건축물의 형상을 구축할 수 있다. 이에 본 연구는 비정형 건축물의 외장재 제작과 시공을 위한 3차원 이미지 스캐닝에 의한 역설계 프로세스와 사례 분석을 통하여 시사점을 도출한다. 본 연구의 결과는 역설계 기술을 사용한 3차원 형상 기술과 설계 요소화 방법을 다양한 건설 프로젝트에 활용할 수 있을 것으로 판단된다.

• 천문학회지
• /
• 제50권6호
• /
• pp.157-165
• /
• 2017

$H_2O$ maser emission at 22 GHz in the circumstellar envelope is one of the good tracers of detailed physics and kinematics in the mass loss process of asymptotic giant branch stars. Long-term monitoring of an $H_2O$ maser spectrum with high time resolution enables us to clarify acceleration processes of the expanding shell in the stellar atmosphere. We monitored the $H_2O$ maser emission of the semi-regular variable R Crt with the Kagoshima 6-m telescope, and obtained a large data set of over 180 maser spectra over a period of 1.3 years with an observational span of a few days. Using an automatic peak detection method based on least-squares fitting, we exhaustively detected peaks as significant velocity components with the radial velocity on a $0.1kms^{-1}$ scale. This analysis result shows that the radial velocity of red-shifted and blue-shifted components exhibits a change between acceleration and deceleration on the time scale of a few hundred days. These velocity variations are likely to correlate with intensity variations, in particular during flaring state of $H_2O$ masers. It seems reasonable to consider that the velocity variation of the maser source is caused by shock propagation in the envelope due to stellar pulsation. However, it is difficult to explain the relationship between the velocity variation and the intensity variation only from shock propagation effects. We found that a time delay of the integrated maser intensity with respect to the optical light curve is about 150 days.

• 한국정보통신학회:학술대회논문집
• /
• 한국해양정보통신학회 2003년도 추계종합학술대회
• /
• pp.995-998
• /
• 2003

MOCVD 법을 이용하여 TiO$_2$ 박막을 제작하여, 투과곡선을 비교적 간단하게 분석할 수 있는 포락선방법을 사용하여 기판온도에 따른 TiO$_2$ 박막의 굴절률, 소광계수 등의 광학적 상수들을 구하였다. 투과곡선의 모사를 실시하여 포락선방법으로 구한 값들이 매우 신뢰도가 높음을 입증하였다. TiO$_2$ 박막은 35$0^{\circ}C$ 에서 부터 결정화가 되기 시작하여, 40$0^{\circ}C$ 이상에서 tetragonal structure 를 갖는 anatase 상으로 완전히 결정화됨을 알 수 있다. 기판온도에 따른 증착률을 Arrhenius plot 하여 구한 활성화에너지는 reaction limited 단계에서 17.8 kcal/mol 이었다. 포락선방법을 이용하여 구한 TiO$_2$ 박막의 굴절률 (λ=632.8 nm) 은 기판온도가 40$0^{\circ}C$ 에서 $600^{\circ}C$ 로 증가함에 따라 2.19 에서 2.32 로 증가하는 추세를 나타내었고, 소광계수는 0.021 에서 0.007로 감소하는 경향을 나타내었다.

• 한국태양에너지학회 논문집
• /
• 제35권4호
• /
• pp.57-66
• /
• 2015

BIPV system not only produces electricity at building, but also acts as a material for building envelope. Thus, it can increase the economical efficiency of PV system by saving the cost for building materials. Bifacial solar cell can convert solar energy to electrical energy from both sides of the cell. In addition, it is designed as 3 busbar layout which is the same with ordinary mono-facial solar cells. Therefore, many of the module manufacturers can easily use the bifacial solar cells without changing their manufacturing equipments. Moreover, bifacial PV system has much potential in building application by utilizing glass-to-glass structure of PV module. However, the electrical generation of the bifacial PV module depends on the characteristics of the building surface which faces the module, as well as outdoor environment. Therefore, in order to apply the bifacial PV module to building envelope as BIPV system, its power generation characteristics are carefully evaluated. For this purpose this study focused on the electrical performance of the bifacial BIPV system through the comparative outdoor experiments. As a result, the power generation performance of the bifacial BIPV system was improved by up to 21% compared to that of the monofacial BIPV system. Therefore, it is claimed that the bifacial BIPV system can replace the conventional BIPV system to improve the PV power generation in buildings.

• 대한기계학회논문집B
• /
• 제20권1호
• /
• pp.266-274
• /
• 1996

An experimental work was conducted to investigate the characteristics of the onset of flooding in vertical annuli with a direct injection mode using air and water. The onset of flooding was determined by means of pressure drop measurement while the air velocity was increased gradually under fixed liquid flow rates. Data of the onset of flooding were collected for various combinations of the tube size and the nozzle number. A theoretical analysis of the onset of flooding was also performed based on an envelope theory. The result shows that the onset of flooding in small-scale annuli can be predicted relatively well by the theory. A modified Wallis parameter was used to investigate the scaling effect of flooding phenomena in the annuli, indicating a relatively reasonable result. The number of nozzle has no effect on the flooding velocity when liquid was injected through 2, 3, 4 and 6 nozzles but the initiation of flooding was significantly expedited when 12 nozzles were employed for liquid injection.

• 천문학논총
• /
• 제30권2호
• /
• pp.219-221
• /
• 2015

We present our recent observations of SDSS J102102.25+174439.9, a new eclipsing white dwarf - main sequence WDMS binary with an orbital period of 0.14 days. This system belongs to the post common-envelope binary group as shown by the spectrum from the Sloan Digital Sky Survey. We obtained our data using the ULTRASPEC instrument installed on the 2.4-m telescope at the Thai National Observatory (TNO). Our multi-band observations reveal an unusual and persistent drop in brightness after the primary eclipse. These dips, which appear to show variations in amplitude, also have a complex shape that changes within days. Dips in WDMS systems have been observed on only one other occasion, in the light curve of QS Vir prior to the eclipse of the white dwarf. The dips in SDSS J1021+1744 are unique because they are present at different wavelengths and they occur approximately at similar phases. Hosting a DA white dwarf and an M4 companion star, this system is known to be the only WDMS to show these kind of dips in its light curve. It is possible that these dips are caused by ejected materials from an active companion star, such as in QS Vir. The light curve in the g' filter exhibits deep and narrow features, implying that the material which passes in front of the white dwarf in SDSS J1021 must be dense and small in size. Furthermore, we try to constrain the stellar and orbital parameters of SDSS J1021+1744 using the Binary Maker 3 software. We use g' and r' data for our light curve analysis to have a better approximation for the red dwarf star.