• Steel and Composite Structures
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• 제48권4호
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• pp.429-441
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• 2023

This research presents an advanced finite element formulation for analyzing the vibratory behaviour of tapered composite shaft rotors, taking into account the impact of the draft angle on the stiffness of the composite shaft laminate. The vibration response of the shaft rotating around its axis is studied using both the finite element hierarchical method and the classical finite element formulation, based on the theory of transverse shear deformation, rotary inertia, gyroscopic effect, and coupling effect due to the stratification of the composite layers of the shaft. The study also includes the development of a program to calculate the Eigen frequencies and critical speeds of the system, and the obtained results are compared with those available in the literature. This research provides valuable insights into the vibratory behaviour of tapered composite shaft rotors and can be useful for designing and optimizing such structures in various industrial applications.

• 한국전자통신학회논문지
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• 제19권2호
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• pp.437-444
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• 2024

회전형 관성항법시스템은 IMU(: Inertial Measurement Unit)를 김블 위에 장착하고 김블을 규칙적으로 회전시켜 IMU의 오차를 상쇄시킴으로써 보다 정확한 항법 정보를 제공할 수 있다. 그러나 파도에 의해 자세 변화가 생기면 회전절차의 한 주기가 끝나는 시점에 자세 오차가 0으로 상쇄되지 않게 되어 큰 위치 오차를 유발한다. 본 논문에서는 이 문제를 고려하여 항체의 롤각 정보를 기반으로 외부 김블을 회전시켜 안정화를 시키는 방법을 제안한다. 시뮬레이션을 기반으로 파도에 의한 영향을 분석하고 외부 김블 안정화의 성능을 검증한다.

• 한국해양공학회지
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• 제30권1호
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• pp.25-31
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• 2016

In this study, hydrodynamic coefficients were obtained from a Rotating Arm (RA) test, which is one of the captive model tests used to provide accurate coefficients in the control motion equation of an underwater vehicle. The RA test was carried out at the RA facility of ADD (Agency for Defense Development), and the forces and moments acting on the underwater vehicle were measured using a six-axis waterproof gage. A multiple regression analysis was used in the analysis of the measured data. The experimental results were also verified by comparison with the theoretical values of the previous linear coefficients. In addition, the stability indices in the horizontal plane were calculated using the linear and nonlinear coefficients, and the dynamic stability of the underwater vehicle was estimated to have a good dynamic performance with a depth ratio of 6.0.

• 대한기계학회논문집B
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• 제26권6호
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• pp.850-858
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• 2002

The present study investigates in detail the combined effects of the Coriolis force and centrifugal force on the development of turbulent flows in a square-sectioned U-bend rotating about an axis parallel to the center of bend curvature. When a viscous fluid flows through a curved region of U-bend, two types of secondary flow occur. One is caused by the Coriolis force due to the rotation of U-bend and the other by the centrifugal force due to the curvature of U-bend. For positive rotation, where the rotation is in the same direction as that of the main flow, both the Coriolis force and the centrifugal force act radially outwards. Therefore, the flow structure is qualitatively similar to that observed in a stationary curved duct. On the other hand, under negative rotation, where these two forces act in opposite direction, more complex flow fields can be observed depending on the relative magnitudes of the forces. Under the condition that the value of Rossby number and curvature ratio is large, the flow field in a rotating U-bend can be represented by two dimensionless parameters : $K_{TC}$ =Re $\sfrac{1}{4}$√λand a body force ratio F=λ/Ro. Here, $K_{TC}$ has the same dynamical meaning as $K_{TC}$ =Re√λ for laminar flow.

• 천문학회보
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• 제41권1호
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• pp.40.1-40.1
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• 2016

Recent integral-field spectrograph surveys have found that similar-looking early type galaxies have wide range of rotational properties (Emsellem et al. 2007). This finding initiated a new point of view to the galaxies; rotation of galaxy as the first parameter of galaxy classification (Emsellem et al. 2011, Cappellari et al. 2011, for example). Some theoretical studies tried to address the origin of galaxy rotation. Idealized galaxy merger simulations have shown that galaxy-galaxy interactions have significant effects on the rotation of galaxies. Cosmological simulations by Naab et al. 2014 also added some more insights to the rotation of galaxies. However, previous studies either lack cosmological background or have not enough number of samples. Running a set of cosmological hydrodynamic zoom-in simulations using the AMR code RAMSES(Teyssier 2002). we have constructed a sample of thousands of galaxies in 20 clusters. Here we present a kinematic analysis of a large sample of galaxies in the cosmological context. The overall distribution of rotation parameter of simulated galaxies suggests a single peak corresponding to fast rotating galaxies. But when divided by mass, we find a strong mass dependency of galaxy rotation, and massive galaxies are distinctively slow rotating. The cumulated effective of mergers seems to neutralize galaxy rotation as suggested by previous studies (Khochfar et al. 2011, Naab et al. 2014, and Moody et al. 2014). This is consistent with the fact that massive galaxies tend to rotate more slowly after numerous mergers. However, if seen individually, merger can either increase or decrease galaxy rotation depending on mass ratio, orbital parameter, and relative rotation axis of the two galaxies. This explains the existence of some non-slow rotating massive early type galaxies.

• 해양환경안전학회지
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• 제18권2호
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• pp.145-152
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• 2012

최근 지구온난화 문제가 대두되면서 신재생에너지 개발을 위한 여러 기술적인 해결책이 제시되고 있는데, 그 중 산업적으로 크게 주목을 받고 있는 분야가 바로 해양에너지이다. 삼면이 바다로 둘러싸인 우리나라는 부존자원이 풍부하여 조력, 조류, 파력에너지에 대한 실용화 기술이 요구되고 있으며, 특히 빠른 조류흐름을 이용하는 조류발전은 해양환경에 거의 영향을 끼치지 않는 친환경적인 발전 방법이다. 조류발전은 조수간만에 의해 발생되는 해수의 자연적인 수평 유체흐름을 로터 및 발전기를 설치하여 회전운동으로 변환시켜 전력을 생산하는 발전 형태이다. 조류발전은 로터의 방향에 따라 크게 수평축 형태와 수직축 형태로 구별할 수 있으며, 발전량은 로터 단면의 크기와 조류속도에 따라 큰차이가 난다. 따라서 본 연구는 저수심형 100 kW급 수평축 조류발전 터빈의 성능해석을 위하여 상용 ANSYS-CFX를 이용하여 3차원 유동해석및 성능평가를 수행하였고, 유동해석을 통해 회전하는 로터 블레이드 표면 유선, 로터 주변 3차원 유동특성에 대해 고찰을 하였다. 그 결과 토크는 터빈의 날개가 증가함에 따라 증가하다가 TSR 3.77에서 최대토크가 발생하였으며, 그 이후 날개끝 속도비가 증가해도 토크는 감소하였다. 또한, 설계유속에서 0.38의 최대 출력계수를 얻었다.

• 한국전산유체공학회지
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• 제13권2호
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• pp.55-61
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• 2008

The Reynolds-Averaged Navier-Stokes(RANS) analysis of the 3-D steady flow around the NREL Phase VI horizontal axis wind turbine(HAWT) rotor was performed. The CFD analysis results were compared with experimental data at several different wind speeds. The present CFD model shows good agreements with the experiments both at low wind speed which formed well-attache flow mostly on the upper surface of the blade, and at high wind speed which blade surface flow completely separated. However, some discrepancy occurs at the relatively high wind speeds where mixed attached and separated flow formed on the suction surface of the blade. It seems that the discrepancy is related to the onset of stall phenomena and consequently separation prediction capability of the current turbulence model. It is also found that strong span-wise flow occurs in stalled area due to the centrifugal force generated by rotation of the turbine rotor and it prevents abrupt reduction of normal force for higher wind speed than the designed value.

• Journal of Power Electronics
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• 제14권1호
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• pp.82-91
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• 2014

This paper proposes a compensation algorithm for the analog rotor position errors caused by nonideal sinusoidal encoder output signals including offset and gain errors. In order to achieve a much higher resolution, position sensors such as resolvers or incremental encoders can be replaced by sinusoidal encoders. In practice, however, the periodic ripples related to the analog rotor position are generated by the offset and gain errors between the sine and cosine output signals of sinusoidal encoders. In this paper, the effects of offset and gain errors are easily analyzed by applying the concept of a rotating coordinate system based on the dq transformation method. The synchronous d-axis signal component is used directly to detect the amplitude of the offset and gain errors for the proposed compensator. As a result, the offset and gain errors can be well corrected by three integrators located on the synchronous d-axis component. In addition, the proposed algorithm does not require any additional hardware and can be easily implemented by a simple integral operation. The effectiveness of the proposed algorithm is verified through several experimental results.

• Journal of Power Electronics
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• 제9권3호
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• pp.343-353
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• 2009

In this paper, a nonlinear controller is proposed for Doubly-Fed Induction Machine (DFIM) drives. The nonlinear controller is designed based on an adaptive backstepping control technique, using a fifth order model of an induction machine in the synchronous d & q axis rotating reference frame, whose d axis coincides with the space voltage vector of the main AC supply, and using the rotor current and stator flux components as state variables. The nonlinear controller can perfectly track the torque reference signal measured in the stator terminals under the condition of unity power factor regulation, in spite of the stator and rotor resistance variations. In order to make the drive system capable of operating in the motoring and generating modes below and above the synchronous speed, two level Space-Vector PWM (SV-PWM) back-to-back voltage source inverters are employed in the rotor circuit. It is confirmed through computer simulation results that the proposed control approach is effective and valid.

• 한국광학회지
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• 제13권2호
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• pp.98-104
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• 2002

비구면 광학부품의 수차 측정 및 성능 평가를 위해 특별 설계된 층밀리기 간섭계를 소개하고, 이와 더불어 층밀리기 간섭계가 갖는 자체의 계통오차를 측정결과로부터 제거하기 위한 보정 방법을 제안한다. 층밀리기 간섭계의 계통오차는 크게 간섭광학계가 갖는 광학오차와 간섭계의 기구부의 불완전에 기인한 층밀리기 방향의 직교오차로 구분할 수 있다. 이들 두 계통 오차들은 모두 본 논문에서 제안하는 방법으로 모두 보정될 수 있다. 보정 방법은 측정 대상물을 간섭계의 광축을 중심으로 회전하여 측정결과로부터 계통오차를 분리하는 자가보정 원리에 근거한다.