• 한국진공학회:학술대회논문집
• /
• 한국진공학회 2014년도 제46회 동계 정기학술대회 초록집
• /
• pp.402.1-402.1
• /
• 2014

Photonic force microscopy (PFM) is an optical tweezers-based scanning probe microscopy, which measures the forces in the range of fN to pN. The low stiffness leads proper to measure single molecular interaction. We introduce a novel photonic force microscopy to stably map various chemical properties as well as topographic information, utilizing weak molecular bond between probe and object's surface. First, we installed stable optical tweezers instrument, where an IR laser with 1064 nm wavelength was used as trapping source to reduce damage to biological sample. To manipulate trapped material, electric driven two-axis mirrors were used for x, y directional probe scanning and a piezo stage for z directional probe scanning. For resolution test, probe scans with vertical direction repeatedly at the same lateral position, where the vertical resolution is ~25 nm. To obtain the topography of surface which is etched glass, trapped bead scans 3-dimensionally and measures the contact position in each cycle. To acquire the chemical mapping, we design the DNA oligonucleotide pairs combining as a zipping structure, where one is attached at the surface of bead and other is arranged on surface. We measured the rupture force of molecular bonding to investigate chemical properties on the surface with various loading rate. We expect this system can realize a high-resolution multi-functional imaging technique able to acquire topographic map of objects and to distinguish difference of chemical properties between these objects simultaneously.

• 대한의용생체공학회:의공학회지
• /
• 제15권4호
• /
• pp.377-382
• /
• 1994

In the conventional Fourier imaging method in MRI (Magnetic Resonance Imaging), intramotion such as pulsatile flow makes zipper-like artifact along the phase encoding direction. On the other hand, line-integral projection reconstruction (LPR) method has advantages such as imaging of short T2, object and reduction of the flow artifact by elimination of the flow-induced phase fluctuation. The LPR, however, necessarily requires time consuming filtering and back-projection processes, so that the reconstruction takes long time. To overcome the long reconstruction time of the LPR and to obtain the flow artifact reduction effect, we adopted phase corrected concentric square raster sampling (CSRS) method and improved its imaging performance. The CSRS is a fast reconstruction method which has the same properties with the LPR. In this paper, we proposed a new method of flow artifact reduction using the CSRS method. Through computer simulations and experiments, we verified that the proposed method can eliminate phase fluctuations, thereby reducing the flow artifact and re- markably shorten the reconstruction time which required long time in the LPR.

• Smart Structures and Systems
• /
• 제17권6호
• /
• pp.935-956
• /
• 2016

With the help of advanced image acquisition and processing technology, the vision-based measurement methods have been broadly applied to implement the structural monitoring and condition identification of civil engineering structures. Many noncontact approaches enabled by different digital image processing algorithms are developed to overcome the problems in conventional structural dynamic displacement measurement. This paper presents three kinds of image processing algorithms for structural dynamic displacement measurement, i.e., the grayscale pattern matching (GPM) algorithm, the color pattern matching (CPM) algorithm, and the mean shift tracking (MST) algorithm. A vision-based system programmed with the three image processing algorithms is developed for multi-point structural dynamic displacement measurement. The dynamic displacement time histories of multiple vision points are simultaneously measured by the vision-based system and the magnetostrictive displacement sensor (MDS) during the laboratory shaking table tests of a three-story steel frame model. The comparative analysis results indicate that the developed vision-based system exhibits excellent performance in structural dynamic displacement measurement by use of the three different image processing algorithms. The field application experiments are also carried out on an arch bridge for the measurement of displacement influence lines during the loading tests to validate the effectiveness of the vision-based system.

• 전자공학회논문지S
• /
• 제35S권7호
• /
• pp.53-61
• /
• 1998

In this paper, we propose an efficient multi-view images coding algorithm to find the optimal depth and texture from the set of multi-view images. The proposed algorithm consists of two consecutive steps, i) the depth estraction step, and ii) the texture extraction step, comparedwith the traditional algorithem which finds the depth and texture concurrently. The X-Y plane of the normalized object space is divided into traingular paatches and the Z value of the node is determined in the first step and then the texture of the each patch is extracted in the second step. In the depth extraction step, the depth of the node is determined by applying the block based disparity compensation method to the windowed area centered at the node. In the second step, the texture of the traingular patches is extracted from the multi-view images by applying the affine transformation based disparity compensation method to the traingular pateches with the depth extracted from the first step. Experimental results show that the SNR(Singnal-to- Noise Ratio) of images enconded by our algorithm is better than that of images encoded by the traditional algorithm by the amount about 4dB for for the test sets of multi-view images called dragon, kid, city and santa.

• 천문학회보
• /
• 제36권1호
• /
• pp.52.1-52.1
• /
• 2011

Black hole masses of Active Galactic Nuclei (AGN) are one of the most important parameters in AGN physics. Based on the virial assumption, black hole masses can be determined from the product of the width of the broad emission lines and the continuum/line luminosities. Using the Low Resolution Imaging Spectrometer(LRIS) at the Keck telescope, we obtained high quality spectra (S/N~100), covering 2300-5500A in the rest-frame, for a sample of 37 intermediate-luminosity AGN at z~0.4, in order to calibrate various black hole mass estimators based on the Mg II (2798A) and the Hbeta (4861A) emission lines. After subtracting continuum and complex FeII emission under Mg II and Hbeta, we fit the broad emission lines using high order Guass-Hermite models to best constrain the profile and the width of the emission lines. Combining the SDSS spectra covering Halpha emission line with the Keck spectra, we determine a set of 6 black hole masses for each object, based on the line width (MgII, Hbeta, and Halpha) and the luminosity (LMgII, LHbeta, LHalpha, L3000, L5100), and calibrate each black hole mass estimator. We will present uncertainties and limitations of each mass estimator.

• 한국분말야금학회:학술대회논문집
• /
• 한국분말야금학회 2006년도 Extended Abstracts of 2006 POWDER METALLURGY World Congress Part 1
• /
• pp.547-548
• /
• 2006

The main object of this research was to examine the effect of sintering conditions on the microstructure of tungsten heavy alloys and how the resulting modification of the microstructure can be used to optimize their mechanical properties. Alloys composed of 88%, 93% and 95% wt. of tungsten and the balance is Ni: Fe in the ratio of 7:3 were sintered at different temperatures for different sintering holding times in hydrogen atmosphere. It was shown that the mechanical properties of the alloys, and especially their ductility, are harmed when tungsten grains are contiguous.

• 한국운동역학회지
• /
• 제13권2호
• /
• pp.175-183
• /
• 2003

The purpose of this study was to analyze the kinetic energy of putter head and ball movements during the process of impact. Highly skilled 5 golfers(less than 1 handicap) participated in this study and the target distance was 3 m. Movements of ball and putter head were recorded with 2 VHS video cameras(60 Hz, 1/500 s shutter speed). Small control object($18.5{\times}18.5{\times}78.5\;cm$) was used in this sdtuldy. Analyzing the process of impact, putter was digitized before 0.0835 s and after 0.0835 s of impact. Ball was digitized 0.1336 s after impact. The results showed that the maximum speed was appeared at Impact and prolonged for a while. Contact point of the club head was within 0.7 cm to the z axis. After contacting the club head, the ball was moved above the ground level(slide) and returned to the ground with sliding and rolling. After contacting the ground, the speed of ball was relied on the surface of the ground. During impact, 70% of kinetic energy of club head has been transferred to the ball.

• 천문학회보
• /
• 제44권1호
• /
• pp.74.3-75
• /
• 2019

Recent Integral Field Spectroscopy (IFS) studies revealed that not only late type galaxies (LTGs) but also early type galaxies (ETGs) have various kinds of kinematic rotation. (e.g. not clearly detectable rotation, disk-like rotation, kinematically distinct core (Cappellari 06)) Among the various studies about galactic kinematics, one of the most notable anomalies is the star-gas misalignment. The gas forms stars and stars release gas through mass-loss. In this process, their angular momentum is conserved. Therefore, kinematic decoupling between stars and gas can occur due to external gas inflow or perturbation of components. There are some possible origins of misalignment: cold gas from filaments, hot gas from outer halo, interaction or merging events with galaxies and environmental effects. Misalignment, the black box from mixture of internal and external gas, can be an important keyword for understanding further about galaxies' kinematics and external processes. Using both SAMI IFS data(Sydney-AAO Multi-object Integral field spectrograph Galaxy Survey, Croom+12) and Horizon-AGN simulation(Dubois+14), we examined misaligned galaxies properties and distribution. Because the simulation has lots of galaxies at various z, we were able to study history of formation, evolution and extinction of misalignment, which was hard to be done with observation only.

• 한국정보과학회논문지:소프트웨어및응용
• /
• 제28권7호
• /
• pp.501-510
• /
• 2001

일반적으로 2D 스테레오 영상으로부터 3차원 모델링을 위해서는 정확한 변위 측정이 필수이다. 기존의 스테레오 영상에서 변위 측정 방식은 전체 영상에 대하여 정합 연산을 수행함으로써 많은 연산 시간과 함께 높은 오 정합 확률의 문제가 있다. 본 논문에서는 스테레오 영상에서의 변위 벡터가 전체 탐색 범위 안에 골고루 분포되어 있지 않고 배경과 물체의 변위에 해당하는 값만을 갖는다는 특성을 이용하여 스테레오 영상을 웨이블릿 변환을 하고 1/4 크기로 줄어든 저주파 영역으로부터 영역 기반 방법을 이용하여 대략적인 변위 영역을 구한다. 대략적인 변위 백터로부터 변위 히스토그램을 생성하고, 이를 이용하여 전경과 배경을 분할 한 뒤, 다시 전경 영상만을 원 영상으로 복원하여 화소의 밝기값이 아닌 2차 미분값을 이용한 화소기반 방법을 통해 조밀한 변위를 구하는 2단계 하이브리드 방법을 제안한다. 또한, 분할된 전경 영역으로부터, 특징점들을 뽑아내고 변위 벡터와 카메라 파라미터를 이용하여 특징점들의 깊이 정보를 추정해 내는 3차원 모델링 과정을 제시한다. 본 논문에서 제안한 방법을 적용할 경우, 기존의 영역 기반 방법의 문제점인 계산 시간 문제를 상당 부분 단축시킬 수 있고, LOG 필터를 통한 2차 미분값을 이용한 화소기반 방법을 추가함으로써, 정밀한 변위를 구할 수 있다. 또한 교차 일치성 검사를 통해 잘못된 변위를 제거하고, 폐색 영역들을 검사할 수 있다. 아울러 3차원 모델링 과정에서, 기존의 Delaunay 삼각측량법의 문제점인 오정합 문제를 전경/배경 분할 알고리즘을 제안함으로써 효과적으로 해결 할 수 있다.

• 대한원격탐사학회지
• /
• 제38권5_1호
• /
• pp.497-510
• /
• 2022

농업용 저수지는 수자원이 계절적으로 편중된 한반도에서 갈수기 용수 공급을 위한 필수적인 구조물이다. 효율적인 물 관리를 위해서는 중소규모 저수지에 대한 체계적이고 효과적인 모니터링이 필요하며, 합성개구 레이더(Synthetic Aperture Radar, SAR) 영상은 전천후 관측이 가능하다는 특징과 함께 연속적인 저수지 모니터링을 위한 도구가 된다. 본 연구에서는 10 m급 해상도를 갖는 Sentinel-1 SAR 영상과 1 m급 해상도의 Capella X-SAR 영상을 활용하여 울산광역시 차리, 갈전, 뒷골 저수지의 수체를 탐지하였으며, 이를 통해 국내 중소규모 저수지 모니터링에의 활용성을 평가하고자 하였다. Z fuzzy function 기반 임계값 산정을 통한 영상분할기법과 객체 탐지 기반 분할기법인 Chan-vese (CV) 기법을 통해 수체 영역을 산정하였으며, UAV 영상과의 비교를 통해 성능을 정량적으로 평가하였다. 임계값 기반 탐지 정확도는 Sentinel-1의 경우 약 0.87, 0.89, 0.77 (차리, 갈전, 뒷골), Capella의 경우 약 0.78, 0.72, 0.81로 나타났으며, CV 기법 적용 시 모든 저수지에서 정확도가 향상되는 것을 확인하였다(Sentinel-1: 0.94, 0.89, 0.84, Capella: 0.92, 0.89, 0.93). Capella는 모든 저수지/분할기법에 대해 수체와 비수체의 경계를 비교적 뚜렷하게 모의하였으나, 고해상도로 인한 speckle noise가 충분히 평활화되지 않아 오탐지 및 미탐지가 다소 발생하였다. 오탐지의 제거를 위해 광학 센서 기반 보조자료를 활용하여 마스킹한 결과, 정확도가 최대 13% 향상되는 것을 확인할 수 있었다. 본 연구 결과를 바탕으로 SAR 위성 기반 더욱 정확한 저수지 탐지가 이루어진다면 소규모 저수지를 포함, 종합적인 가용수량에 대한 연속적인 모니터링이 가능할 것이며, 효과적인 수자원 관리에 기여할 수 있을 것으로 기대된다.