• 한국정보통신학회논문지
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• 제17권7호
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• pp.1558-1563
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• 2013

본 논문에서는 시간영역에서 완전도체 접지평면 위 수직 전기 다이폴에서 방사되는 전자기해석을 통해 전파의 거리에 따른 전파경로손실을 해석하였다. 자유공간에서 수직 전기 다이폴의 해석은 시간영역과 주파수영역에서 많은 연구가 이루어졌으나 본 논문에서는 특히 접지면 위 수직 다이폴을 기지국으로 가정한 전파경로손실특성을 시간영역에서 해석하였으며 접지면의 영향으로 나타나는 근접장의 위치변화와 모바일에서 수신되는 과도응답을 관찰하였다. 본 논문의 결과는 지표면 레이더 및 신호처리 분야에 응용될 수 있을 것이다.

• 로봇학회논문지
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• 제18권4호
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• pp.376-384
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• 2023

In this paper, we introduce an upper extremity rehabilitation robot, NREH (NRC End-effector based Rehabilitation arm at Home). Through NREH, stroke survivors could continuously exercise their upper extremities at home. NREH allows a user to hold the handle of the end-effector of the robot arm. NREH is a end-effector-based robot that moves the arm on a two-dimensional plane, but the tilt angle can be adjusted to mimic a movement similar to that in a three-dimensional space. Depending on the tilting angle, it is possible to perform customized exercises that can adjust the difficulty for each user. The user can sit down facing the robot and perform exercises such as arm reaching. When the user sits 90 degrees sideways, the user can also exercise their arms on a plane parallel to the sagittal plane. NREH was designed to be as simple as possible considering its use at home. By applying error augmentation, the exercise effect can be increased, and assistance force or resistance force can be applied as needed. Using an encoder on two actuators and a force/torque sensor on the end-effector, NREH can continuously collect and analyze the user's movement data.

• 대한전자공학회논문지SP
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• 제39권4호
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• pp.455-461
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• 2002

본 논문에서는 로그폴라 (log-polar) 영상 평면에서의 Hough 변환을 위하여, 잘 알려진 unboundedness 문제를 해결하는 새로운 폴라 형태의 로그 직선 (log line) 매개변수 방정식을 제안한다. 직각 좌표상의 영상으로부터 로그폴라 영상을 생성하기 위하여, 황반부와 주변 영역으로 분리되는 Bolduc의 방법을 이용한다. 그리고 Hough 변환의 입력으로 이용되는 로그폴라 에지 영상은 Sobel 연산자로부터 추출되는 황반부 에지 영상과 본 논문에서 제안하는 공간변형 가중치가 고려된 새로운 그래디언트 연산자가 적용되어 추출되는 주변 영역을 결합하여 생성한다. 그런데 LPM (log-polar mapping; LPM)의 고유한 특성인 비선형 표본화로 인하여 시선고착점으로부터 멀리 떨어진 주변 영역에 포함되는 로그 직선들을 구성하는 화소들은 매우 산재되어 분포된다. 이러한 로그 직선들을 효과적으로 검출하기 위하여 Hough 누적 셀의 값이 공간변형 가중치가 고려되어 계산되도록 한다. 본 논문에서 제안하는 방법이 황반부와 주변 영역을 동시에 지나는 직선들뿐만 아니라 시선고착점으로부터 멀리 떨어진 주변 영역에 존재하는 직선들도 검출될 수 있음을 실험을 통하여 확인한다.

• 디자인학연구
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• 제13권
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• pp.55-64
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• 1996

복식은 조형예술의 한 분야로 인간이 착용함으로써 생명력이 있는 형태를 이루고 인체를 기준으로 하는 입체성을 지닌 공간 조형이다. 그러므로 '옷을 입는다' 라는 단순한 차원을 넘어 인체의 움직임에 의해 나타나는 동감(動感)에 따라 입체적 형태를 이루는 조형성이 복식 디자인의 중요한 요소를 이루게 되었다. 이에 본 연구는 단순한 구조이면서도 인체의 동작과 착장 법에 의해 풍부한 공간감을 살릴 수 있는 관두의를 이론적으로 고찰하였다. 또한 간결하고 현대적인 특징을 지닌 기하학적 도형의 복합 형태 모티브로 한 관두의 형식의 복식 디자인을 연구하였다. 본 연구의 목적은 평면 패턴이 인체에 입혀졌을 때 형성되는 평면성과 입체성의 조화를 추구하며, 착장 법에 의한 기하학적인 면의 자연스러운 분할과 미묘한 색채 및 형태의 구성을 시도하여 보다 더 현대적이며 다양한 가변성(可變性)을 지닌 조형의상을 연구하는데 있다. 작품은 관두의 형식의 T자구조를 토대로 패턴을 구성하여 인체에 직접 입혀 형성되는 조형적 형태를 실험을 통해 실물 작품으로 제작하였다.

• 대한전자공학회논문지SP
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• 제45권3호
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• pp.1-10
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• 2008

점유맵은 3차원 공간상에서 장애물이 놓인 부분과 빈 공간을 구분해서 2차원 평면상에 표현하는 방식으로 자율 내비게이션이나 물체 인식 등을 위해 사용된다. 본 논문에서는 스테레오 영상에서 추출된 깊이 정보를 활용하여 3차원 공간의 점유맵을 구축하고 그 정보를 물체 영역 추출에 활용하는 기법을 제안한다. 스테레오 깊이 영상에서 기반 평면을 추출한 다음, 각 정합점들을 기반 평면 중심 좌표계로 투사하여 점유맵을 추출한다. 본 연구에서는 이렇게 추출된 점유맵을 활용하여 실내외의 다양한 환경에서 움직임 물체 영역을 추출하였는데, 실제 실험 영상을 홍해 제안된 방식의 유용성을 확인한다.

• 대한전기학회:학술대회논문집
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• 대한전기학회 2006년도 제37회 하계학술대회 논문집 C
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• pp.1494-1495
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• 2006

A complete finite element analysis method for discharge onset process, which is governed and coupled by charge transport equation and electric field equation, was presented. The charge transport equation of first order was transformed into a second-order one by utilizing the artificial diffusion scheme. The two second-order equations were analyzed by the finite element formulation which is well-developed for second-order ones. The Fowler-Nordheim injection boundary condition was adopted for charge transport equation. After verifying the numerical results by comparing to the analytic solutions using parallel plane electrodes with one carrier system, we extended the result to blade-plane electrodes in 2D xy geometry with three carriers system. Radius of the sharp tip was taken to be 50 ${\mu}m$. When this sharp geometry was solved by utilizing the space discretizing methods, the very sharp tip was found to cause a singularity in electric field and space charge distribution around the tip. To avoid these numerical difficulties in the FEM, finer meshes, a higher order shape function, and artificial diffusion scheme were employed.

• 로봇학회논문지
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• 제2권2호
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• pp.129-136
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• 2007

This paper introduces a position-based robust visual servoing method which is developed for operation of a human-like robot with two arms. The proposed visual servoing method utilizes SIFT algorithm for object detection and CAMSHIFT algorithm for object tracking. While the conventional CAMSHIFT has been used mainly for object tracking in a 2D image plane, we extend its usage for object tracking in 3D space, by combining the results of CAMSHIFT for two image plane of a stereo camera. This approach shows a robust and dependable result. Once the robot's task is defined based on the extracted 3D information, the robot is commanded to carry out the task. We conduct several position-based visual servoing tasks and compare performances under different conditions. The results show that the proposed visual tracking algorithm is simple but very effective for position-based visual servoing.

• 천문학논총
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• 제28권1호
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• pp.7-13
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• 2013

We present a multi-dimensional reduction method of the surveyed cube database obtained using a single- dish radio telescope in Taeduk Radio Astronomy Observatory (TRAO). The multibeam receiver system installed at the 14 m telescope in TRAO was not optimized at the initial stage, though it became more stabilized in the following season. We conducted a Galactic Plane survey using the multibeam receiver system. We show that the noise level of the first part of the survey was higher than expected, and a special reduction process seemed to be definitely required. Along with a brief review of classical methods, a multi-dimensional method of reduction is introduced; It is found that the 'background' task within IRAF (Image Reduction and Analysis Facility) can be applied to all three directions of the cube database. Various statistics of reduction results is tested using several IRAF tasks. The rms value of raw survey data is 0.241 K, and after primitive baseline subtraction and elimination of bad channel sections, the rms value turned out to be 0.210 K. After the one-dimensional reduction using 'background' task, the rms value is estimated to be 0.176 K. The average rms of the final reduced image is 0.137 K. Thus, the image quality is found to be improved about 43% using the new reduction method.

• 천문학회보
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• 제45권1호
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• pp.46.3-47
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• 2020

Variations in the brightness of asteroids are caused by their spins, irregular shapes and companions. Thus, in principle, the spin state and shape model of a single object or, a combined model of spins, shapes and mutual orbit of a multiple components can be constructed from the analysis of light curves obtained from the time-series photometry. Using ground- and space-based facilities, a number of time-series photometric observations of asteroids have been conducted to find the possible causes of their light variations. Nonetheless, only about 2% of the known asteroids have been confirmed for their rotation periods. Therefore, a follow-on systematic photometric survey of asteroids is essential. We started an asteroid light curve survey for this purpose using Korea Microlensing Telescope Network (KMTNet) during 199 nights between the second half of 2019 and the first half of 2020. We monitored within a 2° × 14° region of the sky per each night with 25 min cadences. In order to observe as many asteroids as possible with a single exposure, we mostly focus on the ecliptic plane. In our survey, 25,925 asteroids were observed and about 8,000 of them were confirmed for their rotation periods. In addition, using KMTNet's 24-hour continuous monitoring, we collected many composite light curves of slow rotating asteroids that were rarely obtained with previous observations. In this presentation, we will introduce the typical light curves of asteroids obtained from our survey and present a statistical analysis of spin states and shapes of the asteroids from this study.

• 한국우주과학회:학술대회논문집(한국우주과학회보)
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• 한국우주과학회 2008년도 한국우주과학회보 제17권2호
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• pp.27.1-27.1
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• 2008

KASI (Korea Astronomy and Space Science Institute) is developing a compact wide-field survey space telescope system, MIRIS (The Multi-purpose IR Imaging System) to be launched in 2010 as the main payload of the Korea Science and Technology Satellite 3. Through recent System Design Review (SDR) and Preliminary Design Review (PDR), most of the system design concept was reviewed and confirmed. The near IR imaging system adopted short F/2 optics for wide field low resolution observation at wavelength band 0.9~2.0 um minimizing the effect of attitude control system. The mechanical system is composed of a cover, baffle, optics, and detector system using a $256\times256$ Teledyne PICNIC FPA providing a $3.67\times3.67$ degree field of view with a pixel scale of 51.6 arcsec. We designed a support system to minimize heat transfer with Muti-Layer Insulation. The electronics of the MIRIS system is composed of 7 boards including DSP, control, SCIF. Particular attention is being paid to develop mission operation scenario for space observation to minimize IR background radiation from the Earth and Sun. The scientific purpose of MIRIS is to survey the Galactic plane in the emission line of Pa$\alpha$ ($1.88{\mu}m$) and to detect the cosmic infrared background (CIB) radiation. The CIB is being suspected to be originated from the first generation stars of the Universe and we will test this hypothesis by comparing the fluctuations in I (0.9~1.2 um) and H (1.2~2.0 um) bands to search the red shifted Lyman cutoff signature.