• 한국군사과학기술학회지
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• 제22권5호
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• pp.674-686
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• 2019

In this paper, we will discuss the absolute angular error control mode for the Gun/Turret driving system. The Gun/Turret driving controller receives absolute angular error calculated from the fire control system (FCS). Thus, the Gun/Turret driving controller is subjected to step command to cause residual vibration and system unstable. In order to reduce residual vibration and to ensure the system stability, we propose an error motion profile method with two types of trapezoidal and S-Curve. The validity of the proposed error motion profile method is confirmed via simulation by observing that the resulting position error, driving power, and power density satisfied the control performance.

• 한국전자통신학회논문지
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• 제14권4호
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• pp.645-650
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• 2019

본 논문에서는 기존의 l=1 궤도 각운동량 모드에 대해서만 연구가 이루어지던 광 도파로 구조를 개선하여 반도체 박막 공정으로 제작이 가능하고, l=1 및 l=2 궤도 각운동량 모드를 전송할 수 있는 광 집적회로용 실리콘 광 도파로를 유한차분법을 통하여 설계하였다. 설계된 광 도파로는 여러 층의 실리콘과 실리콘 산화막으로 이루어져 있으며, 두 고유 모드의 합성을 통하여 궤도 각운동량을 가지는 모드를 구현한다. 제안된 광 도파로의 2차 궤도 각운동량 모드의 전기장 분포를 통한 궤도 각운동량 계산 결과, 궤도 각운동량 양자수가 1차 및 2차 각각 l= 0.9642, 1.8766으로 이론치에 매우 근접한 값을 보였다.

• 대한전자공학회논문지SD
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• 제37권11호
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• pp.36-42
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• 2000

Buried channel waveguides의 필드 분포에 대한 analytic 표현식을 effective index method (EIM), variational method(VM)와 각각의 방향으로의 경계조건을 적용한 variational method (VM_vec)를 사용하여 구한 뒤 angular spectrum 방법을 적용하여 도파로 폭에 따른 단면 반사율을 계산하고 이를 비교 검토하였다. 도파로 폭이 커질수록 buried channel waveguides의 단면 반사율은 slab 도파로의 단면 반사율에 접근하였고 도파로 폭이 작아질수록 slab 도파로의 단면 반사율로부터 quasi-TE 모드의 단면 반사율은 감소하였고 quasi-TM 모드의 단면 반사율은 증가하였다. 도파로 폭에 따른 단면 반사율 변화량은 quasi-TM 모드보다 quasi-TE 모드에 대한 변화량이 크게 나타남을 알 수 있었다. Aspect ratio가 1일 때 VM과 VM_vec으로 구한 quasi-TE 모드와 quasi-TM 모드와 quasi-TM 모드의 반사율은 차이가 크게 나타났다. Quasi-TE 모드의 경우는 VM_vec으로 구한 필드 분포에 angular spectrum 방법을 적용하여 계산한 단면 반사율이 EIM으로 구한 반사율보다 정확한 값임을 알 수 있었고 quasi-TM 모드의 경우는 각 방법으로 구한 반사율이 거의 같음을 볼 수 있었다.

• 한국소음진동공학회논문집
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• 제16권9호
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• pp.912-918
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• 2006

A modeling method for the vibration analysis of rotating multi-blade systems considering the coupling stiffness effect is presented in this paper. Blades are assumed as cantilever beams and the coupling stiffness effect originates from disc or shroud between blades. As the angular speed, hub radius ratio, and the coupling stiffness vary, the natural frequencies of the system vary. Numerical results show that the coupling stiffness is very important to estimate the natural frequencies. Along with the natural frequencies, associated mode shapes, critical angular speed, and critical hub radius ratio are obtained through the analysis.

• 한국소음진동공학회:학술대회논문집
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• 한국소음진동공학회 2006년도 춘계학술대회논문집
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• pp.1354-1359
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• 2006

A modeling method for the vibration analysis of rotating multi-blade systems considering the coupling stiffness effect is presented in this paper. Blades are assumed as cantilever beams and the coupling stiffness effect originates from disc or shroud between blades. As the angular speed, hub radius ratio, and the coupling stiffness vary, the natural frequencies of the system vary. Numerical results show that the coupling stiffness is very important to estimate the natural frequencies. Along with the natural frequencies, associated mode shapes, critical angular speed, and critical hub radius ratio are obtained through the analysis.

• Journal of Welding and Joining
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• 제6권3호
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• pp.21-26
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• 1988

The behavior of angular distortion in butt joint wleding of thin plate structure is investigated with an experimental model and partially with a computational model. The experimental model studying the effects of specimene size and degree of restraint on the angular distorion offers a good method for analyzing the behavior of the distrotion. In addition, the distrotion during welding was demonstrated by both experimental measurement and numericla prediciton. The facts evealed in this study are as follows : 1) distrotion angles were changed with variations of specimene wldth. 2) With the restraint, angular distrotion was reduced to 20% to that of free joint. 3) After the restraint being removed, the effect of restraint was also remained. 4) Same heat input per unit thickness caused same amount of distortion. 5) The mode of angular distortion was expected to be changed with expected to be changed with time, i.e. convex movement during heating and concave one during cooling.

• 한국정밀공학회:학술대회논문집
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• 한국정밀공학회 2012년도 추계학술대회 논문집
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• pp.305-306
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• 2012

• 한국통신학회논문지
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• 제8권4호
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• pp.164-171
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• 1983

본 논문에서는 비교적 짧은 계단형 멀티모우드 광섬유를 이용하여 여러 정보의 채널을 전송하는 광멀티플렉싱 기술인 각도분할방식(ADM: Angular Division Multiplexing)에 대해 논하였다. 평면파 입력에 대한 광섬유 내의 모우드 결합과 출력 파워 분포가 계산되었으며 시스템의 혼신도 결정이 제시되었다. 모우드 결합 하에서 광섬유의 길이와 입력조건에 따른 펄스폭이 평면 도파판과 광섬유에 대해 비교, 계산되었다. NA(Numerical Aperture)아래의 입력각에 대한 각도폭은 입력각이 클수록 줄어들었으며 출력은 입력각에 파워가 집중된 환형으로 나타났으며 이는 ADM시스템의 중요한 요인이 되었다.

• 제어로봇시스템학회논문지
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• 제20권5호
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• pp.563-569
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• 2014

This article focuses on a hemispherical resonator gyro driven by the Coriolis effect. A hemispherical shell, called a resonator, is maintained in the resonance state by amplitude control and phase locking control. Parametric excitation has been used to control the amplitude. For rate measurement mode or FTR mode, nodal points have been kept to an amplitude of zero. Angular rate measurement has been demonstrated by rotating a resonator. Frequency mismatch between two stiffness principal axes is a major cause of low performance: vibrating pattern drift and reduced control effectiveness. This mismatch has been reduced significantly by the addition of small mass. A negative spring effect, which lowers resonance frequencies, has been verified experimentally.

• 천문학회보
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• 제36권1호
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• pp.47.2-47.2
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• 2011

Gravitational waves from the pulsar glitch can be detected by next generation gravitational wave observatories. We investigate characteristics of the modes that can emit the gravitational waves excited by three different types of perturbations satisfying conservation of total rest mass and angular momentum. These perturbations mimic the pulsar glitch theories i.e., change of moment of inertia due to the star quakes or angular momentum transfer by vortex unpinning at crust-core interface. We carry out numerical hydrodynamic simulations using the pseudo-Newtonian method which makes weak field approximation for the dynamics, but taking all forms of energies into account to compute the Newtonian potential. Unlike other works, we found that the first and second strongest modes that give gravitational waves are $^2p_1$ and $H_1$ rather than$^2f$. We also found that vortex unpinning model excites the inertial mode in quadrupole moment quite effectively. The inertial mode may evolve into the non-axisymmetric r-mode.