• 대한치과보철학회지
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• 제8권1호
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• pp.133-135
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• 1968

주의(主意)깊게 계획(計劃)되고 제작(製作)된 guiding planes을 가진 국소의치(局所義齒)는 약화(弱化)된 치아(齒牙)를 안정(安靜)시키는데 효과적(效果的)이다. 설계(設計)에 있어서 중요(重要)한 요소(要素)들고 이러한 수부물(修復物)의 적합법(適合法)을 기술(記述)하였다.

• 한국광학회:학술대회논문집
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• 한국광학회 2000년도 제11회 정기총회 및 00년 동계학술발표회 논문집
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• pp.146-147
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• 2000

The electromagnetic wave scattering from active objects has only recently attracted attention.$^{(1).(3)}$ Theoretical studies have considered normal-incidence plane-wave interactions with active dielectric cylinders with the prediction of large enhancements in the scattered field for bound mode structures. According to the theory of the electromagnetic wave scattering from a dielectric cylinder, the eigenvector solutions are discrete and have both guided (non-radiative) and leaky (radiative) mode solutions. By using an anti-guiding (leaky) structure instead of a guided structure and scattering at oblique incident angles near critical angle, the scattering resonances predicted by theoretical studies were obtained for the first time. A fine-grained scan of the plane-wave incident angle a reveals the existence of discrete scattering resonances. The diameter and real part of the index of refraction determine the resonant conditions and the imaginary part of the refractive index has a threshold value to make mode up for its radiation loss. The cross coupling between transverse electric (TE) and transverse magnetic (TM) modes is clearly detected for both active and passive scattering as theoretically expected. (omitted)

• 천문학회보
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• 제38권2호
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• pp.82.1-82.1
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• 2013

The SPICA (SPace Infrared Telescope for Cosmology & Astrophysics) project is a next-generation infrared space telescope optimized for mid- and far-infrared observation with a cryogenically cooled 3m-class telescope. Owing to unprecedented sensitivity and high spatial resolution, the focal plane instruments are expected to perform the confusion-limited observation. The SPICA will challenge to reveal many astronomical key issues from the star-formation history of the universe to the planetary formation. The Korean 5contribution to SPICA as an international collaboration is the development of the near-infrared instrument, FPC (Focal Plane Camera). The Korean consortium for FPC proposed a key system instrument for the purpose of a fine guiding (FPC-G) complementing the AOCS (Attitude and Orbit Control System). The back-up instrument of FPC-G, FPC-S will be responsible for the scientific observations as well. Through the international review process, we have revised the scientific programs and made the feasibility study for the fine guiding system. Here, we report the current status of SPICA/FPC project.

• Journal of Biosystems Engineering
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• 제24권3호
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• pp.209-216
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• 1999

A self-travelling sprayer was developed to avoid the exposure of an operator to agricultural chemicals and exhaust gas, to improve safety and to increase working efficiency during the application and transport work in the greenhouses. This system consists of self-travelling system and the control system for application and safety device. The auto-spray car is equipped with a liquid chemical tank of 80l capacity. The travelling system adopted mechanical steering system which link mechanism of front wheel is guided by guide rollers. The sprayer travels along the guiding pipe which is set on the furrow in the greenhouses. The sprayer stops automatically applying and traveling when the liquid chemical tank becomes empty or when the sprayer reach the turning point. The spray booms swings in a vertical plane. The control system of safety devices controls the automatic stop of the sprayer when there is an obstacle on the traveling path, or when the battery becomes discharged. The auto-spray car traveled smoothly and steadily along the guide pipe during traveling straightly and turning on the ground.

• 한국컴퓨터그래픽스학회논문지
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• 제25권3호
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• pp.31-41
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• 2019

포그 스크린은 미세한 물방울들로 구성된 스크린으로 관찰자는 포그 스크린을 투과한 영상을 관찰하게 된다. 일반 스크린과는 달리 관찰자는 무대 위에서 연기자가 포그 스크린에 표시된 이미지를 뚫고 들어가는 모습을 볼 수 있다. 본 논문에서는 상부에서 생성된 포그 입자 집단이 중력에 의하여 아래로 떨어질 때 평평한 수직 스크린을 이루도록 하는 하향식 포그 스크린 생성 장치 구현 방법을 기술한다. 본 기법은 수조안에 배치된 초음파 진동자에 의해 수조 표면에서 포그 입자가 발생되는 원리를 이용한다. 생성된 포그 집단이 하나의 평면을 유지할 수 있도록 포그가 나오는 통로 출구 양옆에 가이드 바람을 형성하는 기법과 포그 스크린 생성 장치의 설계와 제작 방법을 기술한다.

• 천문학회지
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• 제51권6호
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• pp.207-214
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• 2018

A coelostat is often used for solar observations, because it corrects the image rotation automatically by guiding sunlight into a fixed telescope with two plane mirrors. For the purposes of education and spectroscopic observation, the solar group at Seoul National University (SNU) plans to develop the SNU coelostat (SNUC) and install it in the SNU Astronomical Observatory (SAO). Requirements of the SNUC are < 1" positioning accuracy with 30 cm beam size on the entrance pupil in the compact dome. To allow for installation in the small dome, we design a compact slope type coelostat with a 45 cm primary plane mirror and a 39 cm secondary plane mirror. The motion of the SNUC is minimized by fixing the position of the slope frame. Numerical simulations of the available observational time of the designed coelostat shows that the sun can be observed ay all times from June to early August and at least three hours in other months. Since the high accuracy driving motors installed in the SNUC can be affected by external environment factors such as humidity and temperature variations, we design a prototype to test the significance of these effects. The prototype consists of a 20 cm primary plane mirror, a 1 m slope rail, a direct drive motor, a ballscrew, a linear motion guide, an AC servo motor, a reduction gear and a linear encoder. We plan to control and test the accuracy of the prototype with varying atmospheric conditions in early 2019. After testing the prototype, the SNUC will be manufactured and installed in SAO by 2020.

• 한국컴퓨터산업학회논문지
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• 제2권12호
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• pp.1609-1616
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• 2001

본 논문에서는 체적 홀로그램을 이용한 무안경 3차원 디스플레이 시스템을 제안하였다. 디스플레이 평면에서 다시점 스테레오 영상을 관찰할 수 있도록 각 다중화된 기준파와 물체파를 간섭시킨 후 격자 패턴을 체적홀로그램에 기록하였다. 디스플레이 하고자 하는 다안식 영상으로 구성된 물체파가 시분할적으로 update 되며 광굴절 매질에 입사될 때 브래그 조건을 만족시키면, 출력 평면에서는 회절된 영상으로부터 다안식 3차원 영상을 관찰할 수 있다. 본 시스템을 이용함으로써 시점의 증가에 따른 해상도의 저하가 없는 고해상 다시점 3차원 디스플레이를 구성할 수 있다.

• 유체기계공업학회:학술대회논문집
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• 유체기계공업학회 2006년 제4회 한국유체공학학술대회 논문집
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• pp.291-294
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• 2006

Exhaust system of steam turbines consists of an annular diffuser and a collector and connects the last stage turbine and the condenser. The system is used to transfer the turbine leaving kinetic energy to potential energy while guiding the flow from turbine exit plane to the downstream condenser. In the steam turbine exhaust system, distorted pressure profile is arisen by the nonaxisymmetric collector structure at the diffuser outlet, and this distorted pressure is propagated to the last stage LP turbine exit plane through the diffuser, then the last stage LP turbine experiences asymmetric back pressure. It is known that the pressure recovery performance of diffuser is strongly influenced by diffuser inflow condition. In this study, the effect of exhaust system due to the changing of inlet flow condition is observed by using CFD, and the interaction of last stage LP turbine and exhaust system is investigated by using actuator disk model as modeling of turbine blade row of exhaust hood inlet.

• 한국통신학회논문지
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• 제37권8A호
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• pp.698-705
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• 2012

무안경 방식 스테레오스코픽 입체 디스플레이 시스템에서 시역간 크로스토크는 입체시를 저해하는 주요 문제이다. 기존 크로스토크에 대한 연구는 관찰자면에서 수평 방향으로 인접한 시역간 겹침비를 정량적으로 분석하는 것이 대부분이었으나, 본 연구에서는 이를 포함, 깊이 방향으로 형성되는 해당시점영상의 밝기분포를 정량화하여 수평, 깊이방향에 따른 유효 관찰영역을 제시함으로서 효과적인 입체시 시청 범위를 제공하는데 목적을 두었다. 본 논문에서는 무안경방식의 스테레오스코픽 입체 디스플레이 환경에서 유발되는 크로스토크의 주요 인자들을 디스플레이 환경 및 관찰환경에서 도출하고 이들의 관계를 정성적으로 분석할 수 있는 알고리듬 개발 및 이를 가시화 할 수 있는 시뮬레이션 툴을 제작하였다. 더불어 시뮬레이션 결과를 응용하여 관찰자를 최적의 입체시 시청영역으로 유도 할 수 있는 최적입체시 가이드 시스템을 제안하였다.

• 천문학회보
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• 제38권1호
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• pp.76.2-76.2
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• 2013

SPICA(SPace Infrared Telescope for Cosmology and Astrophysics) is an infrared space observatory with cooled telescope of 3 m aperture. Because of its large aperture, near- and mid-infrared instruments onboard SPICA require fine guidance with attitude accuracy less than 0.1 arcsecond. The FPC-G is a focal plane camera to achieve this high attitude accuracy and KASI is leading its development. The SPICA project is now under the Risk Mitigation Phase 2 (RMP2) and one of major risks is to satisfy the requirement of pointing and attitude control. To assess the impacts of disturbance sources on the attitude control and devise methods to mitigate possible risks, a software simulator of the FPC-G is under the development. In this presentation, we report the status of development of the simulator and the development plan during the RMP2.