• KIEE International Transaction on Electrical Machinery and Energy Conversion Systems
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• 제2B권3호
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• pp.125-132
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• 2002

PMSMS (permanent magnet synchronous motors) are widely used in industrial applications and home appliances because of their high torque to inertia ratio, superior power density, and high efficiency. For high performance control, accurate informations about the rotor position is essential. Sensorless algorithms have lately been studied extensively due to the high cost of position sensors and their low reliability in harsh environments. A novel position sensorless speed control for PMSMs uses indirect flux estimation and is presented in this paper. Rotor position and angular velocity are estimated by the proposed indirect flux estimation. Linkage flux and magnetic field flux are calculated by the voltage equations and the measured phase current without any integration. Instead of linkage flux calculation with integral operation, indirect flux and differential magnetic field are used for the estimation of rotor position. A proper rejection technique fur current noise effect in the calculation of differential linkage flux is introduced. The proposed indirect flux detecting method is free from the integral rounding error and linkage flux drift problem, because differential linkage flux can be calculated without any integral operation. Furthermore, electrical parameters of the PMSM can be measured by the proposed TCM (time compression method) for soft starting and precise estimation of rotor position. The position estimator uses accurate electrical parameters that are obtained from the proposed TCM at starting strategy. In the operating region, a proper compensation method fur temperature effect can compensate fir the estimation error from the variation of electrical parameters. The proposed novel position sensorless speed control scheme is verified by the experimental results.

• 한국통신학회논문지
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• 제28권11C호
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• pp.1111-1117
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• 2003

이동 통신 시스템에서 이동체의 속도 추정은 수신신호의 최대 도플러 주파수를 찾는 과정이다. 하지만 실제적인 이동 통신 환경에서 이동체의 속도 추정은 부가된 잡음의 영향으로 많은 왜곡을 가지게 된다. 본 논문에서는 이동 통신 환경에서 최대 도플러 주파수 추정 시 부가 잡음의 영향을 억제하기 위한 결정 궤환 적응형 대역 제한(Decision Feedback Doppler Adaptive Band-Limit : DF-DABL) 알고리즘을 제안한다. 제안된 알고리즘에서는 잡음의 2차 통계 특성을 대역 제한 방법을 통하여 신호의 특성과 일치하게 함으로서 부가된 잡음의 영향을 효과적으로 제거한다. 특히 제안된 방법에서는 신호대잡음비 (SNR)와 같은 추가 채널 정보를 필요로 하지 않는다.

• 자동차안전학회지
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• 제5권2호
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• pp.17-23
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• 2013

This paper describes an algorithm for Advanced Emergency Braking(AEB) with tire-road friction coefficient estimation. The AEB is a system to avoid a collision or mitigate a collision impact by decelerating the car automatically when forward collision is imminent. Typical AEB system is operated by Time-to-collision(TTC), which considers only relative velocity and clearance from control vehicle to preceding vehicle. AEB operation by TTC has a limit that tire-road friction coefficient is not considered. In this paper, Tire-road friction coefficient is also considered to achieve more safe operation of AEB. Interacting Multiple Model method(IMM) is used for Tire-road friction coefficient estimation. The AEB algorithm consists of friction coefficient estimator and upper level controller and lower level controller. The numerical simulation has been conducted to demonstrate the control performance of the proposed AEB algorithm. The simulation study has been conducted with a closed-loop driver-controller-vehicle system using using MATLAB-Simulink software and CarSim Vehicle model.

• ETRI Journal
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• 제33권4호
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• pp.487-496
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• 2011

Korea Multi-Purpose Satellite-5 (KOMPSAT-5) is the first satellite in Korea that provides 1 m resolution synthetic aperture radar (SAR) images. Precise orbit determination (POD) using a dual-frequency IGOR receiver data is performed to conduct high-resolution SAR images. We suggest orbit determination strategies based on a differential GPS technique. Double-differenced phase observations are sampled every 30 seconds. A dynamic model approach using an estimation of general empirical acceleration every 6 minutes through a batch least-squares estimator is applied. The orbit accuracy is validated using real data from GRACE and KOMPSAT-2 as well as simulated KOMPSAT-5 data. The POD results using GRACE satellite are adjusted through satellite laser ranging data and compared with publicly available reference orbit data. Operational orbit determination satisfies 5 m root sum square (RSS) in one sigma, and POD meets the orbit accuracy requirements of less than 20 cm and 0.003 cm/s RSS in position and velocity, respectively.

• 대한전자공학회논문지TC
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• 제37권7호
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• pp.9-17
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• 2000

마이크로셀 구조에서 효율적으로 핸드오프와 채널 할당을 수행하기 위하여 이동체의 위치 및 속도를 추정 하는 것이 중요한 문제로 대두되고 있다. 이전 연구에서, 마이크로셀 환경에서 응용할 수 있는 이동체의 위치 추정 방법을 제안했다. 제안된 방법은 탐색 지역을 단계적으로 좁혀서 이동체가 위치한 지역을 결정하는 3단계 위치 추정 방법에 근거한다. 3단계 위치 추정 방법을 사용하여, 섹터 추정 단계에서 섹터를 추정하고, 트랙 추정 단계에서는 트랙을, 최종적으로 블럭 추정 단계에서 이동체가 위치한 블럭을 추정한다. 그러나 이 방법은 이동체가 섹터나 트랙의 경계 지점에 위치할 경우 추정의 정확도가 감소되는 문제점이 있다. 본 연구에서는 가상구역 개념을 이용하여, 경계 지역에 있는 이동체에 대한 추정 오류율을 줄일 수 있는 위치추정 방법을 제안한다.

• 천문학회보
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• 제46권2호
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• pp.67.4-68
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• 2021

In studying the dynamical evolution of galaxy clusters, one intriguing approach is to compare the spatial distributions of various components, such as the dark matter, the member galaxies, the gas, and the intracluster light (ICL; the diffuse light from stars, which are not bound any individual cluster galaxy). If we find a visible component whose spatial distribution coincides with the dark matter distribution, then we could draw a dark matter map without requiring laborious weak lensing analysis. Furthermore, if the component traces the dark matter distribution better for more relaxed galaxy cluster, we could use the similarity as a dynamical stage estimator of the galaxy cluster. We present a novel new methodology to quantify the similarity of two or more 2-dimensional spatial distributions. We apply the method to a sample of galaxy clusters at different dynamical stages simulated within N-cluster Run, which is an N-body simulation using the galaxy replacement technique. Among the various components (stellar particles, galaxies, ICL), the velocity defined ICL+ brightest cluster galaxy (BCG) component traces the dark matter best. Between the sample galaxy clusters, the relaxed clusters show stronger similarity of the spatial distribution between the dark matter and ICL+BCG than the dynamically young clusters.

• 한국전자통신학회논문지
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• 제6권6호
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• pp.855-864
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• 2011

본 논문은 IPMSM(Interior Permanent Magnet Synchronous Motor)의 고성능 운전을 위해 비선형 제어를 기반으로 하는 적응 백스텝핑 제어기를 제안한다. 먼저 각속도의 추종성능을 향상시키기 위해서 비선형 백스텝핑 제어기를 설계한다. 파라메타 변동의 영향을 고려하지 않고 설계된 제어기는 고성능 운전이 어렵다. 부하토크의 변동에 대해 실시간 적응할 수 있는 파라메타 추정기를 설계에 포함하여 고성능 운전이 가능하게 한다. 또한 전동기의 효율적인 전력소비를 위하여 최대토크를 얻기 위한 최소전류의 운전을 할 수 있도록 제어기를 설계하였다. 제안된 제어기로 2마력급의 IPMSM에 적용하여 각속도 레퍼런스에 대한 추종성능과 부하토크 변동에 대한 추정, 그리고 MTPA(Maximum Torque per Ampere) 운전을 시험하여 일정토크 운전영역에서 안정화된 강건한 제어기임을 시뮬레이션을 통해 확인할 수 있었다.

• 제어로봇시스템학회논문지
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• 제20권7호
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• pp.767-773
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• 2014

The carrier-to-noise power ratio is a key parameter for determining the reliability of PVT (Position, Velocity, and Time) solutions which are obtained by a GNSS (Global Navigation Satellite System) receiver. It is also used for locking a tracking loop, deciding the re-acquisition process, and processing advanced navigation in the receiver subsystem. The representative carrier-to-noise power ratio estimation schemes are the narrowband-wideband power ratio method (NW), the MM (Moment Method), and Beaulieu's method (BL). The NW scheme is the most classical one for commercial GNSS receivers. It is often used as an authoritative benchmark for assessing carrier-to-noise power estimation schemes. The MM scheme is the least biased solution among them, and the BL scheme is a simpler scheme than the MM scheme. This paper focuses on the less biased estimation with low complexity when the residual phase noise remains, then proposes a novel carrier-to-noise power ratio estimation scheme with low complexity for GNSS receivers. The asymptotic bias of the proposed scheme is derived and compared with others, and the simulation results demonstrate that the complexity of the proposed scheme is lowest among them, while the estimation performance of the proposed scheme is similar to those of the BL and MM schemes in normal and high gained reception environments.

• 천문학회보
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• 제35권2호
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• pp.49.1-49.1
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• 2010

The study of pores, small penumbraless sunspots, can give us a chance to understand how strong magnetic fields interact with convective motions in the photosphere. For a better understanding of this interaction, we investigate the temporal variation of several tiny pores smaller than 2". These pores were observed by the Solar Optical Telescope (SOT) onboard Hinode on 2006 December 29. We have analyzed the high resolution spectropolarimetric (SP) data and the G-band filtergrams taken during the observation. Magnetic flux density and Doppler velocities of the pores are estimated by applying the center of gravity (COG) method to the SP data. The horizontal motions in and around the pores are tracked by adopting the Nonlinear Affine Velocity Estimator (NAVE) method to the G-band filter images. As results, we found the followings. (1) Darkness of pores is positively correlated with magnetic flux density. (2) Downflows always exist inside and around the pores. (3) The speed of downflows inside the pores is negatively correlated with their darkness. (4) The pores are surrounded by strong downflows. (5) Brightness changes of the pores are correlated with the divergence of mass flow (correlation coefficient > 0.9). (6) The pores in the growing phase are associated with the converging flow pattern and the pores in the decay phase with the diverging flow pattern. Our results support the idea that a pore grows as magnetic flux density increases due to the convergence of ambient mass flow and it decays with the decrease of the flux density due to the diverging mass flow.

• 한국운동역학회지
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• 제23권1호
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• pp.53-62
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• 2013

The methods of fitting a circle to measured data, geometric fit and algebraic fit, have been studied profoundly in various areas of science. However, they have not been applied exactly to a biomechanics discipline for locating the center of rotation of a human joint. The purpose of this study was to generalize the methods to fitting spheres to the points in 3-dimension, and to estimate the center of rotation of a hip joint by three of geometric fit methods(Levenberg-Marquardt, Landau, and Sp$\ddot{a}$th) and four of algebraic fit methods(Delogne-K${\aa}$sa, Pratt, Taubin, and Hyper). 1000 times of simulation experiments for flexion/extension and ad/abduction at an artificial hip joint with four levels of range of motion(10, 15, 30, and $60^{\circ}$) and three levels of angular velocity(30, 60, and $90^{\circ}$/s) were executed to analyze the responses of the estimated center of rotation. The results showed that the Sp$\ddot{a}$th estimate was very sensitive to the marker near the center of rotation. The bias of Delogne-K${\aa}$sa estimate existed in an even larger range of motion. The Levenberg-Marquardt algorithm of geometric fit and the Pratt of algebraic fit showed the best results. The combination of two methods, using the Pratt's estimate as initial values of the Levenberg-Marquardt algorithm, could be a candidate of more valid estimator.