• IUGG한국위원회:학술대회논문집
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• IUGG한국위원회 2003년도 정기총회 및 학술발표회
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• pp.14-14
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• 2003

SAR (Synthetic Aperture Radar) is an imaging radar which can scan and image Earth System targets without solar illumination. Most Earth observation Shh systems operate in X-, C-, S-, L-, and P-band frequencies, where the shortest wavelength is approximately 1.5 cm. This means that most opaque objects in the SAR signal path become transparent and SAR systems can image the planetary surface targets without sunlight and through rain, snow and/or even volcanic ash clouds. Most conventional SAR systems in operation, including the Canada's RADARSAT-1, operate in one frequency and in one polarization. This has resulted in black and with images, with which we are familiar now. However, with the launching of ENVTSAT on March 1 2002, the ASAR system onboard the ENVISAT can image Earth's surface targets with selected polarimetric signals, HH+VV, HH+VH, and VV+HV. In 2004, Canadian Space Agency will launch RADARSAT-II, which is C-band, fully polarimetric HH+VV+VH+HV. Almost same time, the NASDA of Japan will launch ALOS (Advanced land Observation Satellite) which will carry L-band PALSAR system, which is again fully polarimetric. This means that we will have at least three fully polarimetric space-borne SAR system fur civilian operation in less than one year. Are we then ready for this new all weather Earth Observation technology\ulcorner Actual imaging process of a fully polarimetric SAR system is not easy to explain. But, most Earth system scientists, including geologists, are familiar with polarization microscopes and other polarization effects in nature. The spatial resolution of the new generation of SAR systems have also been steadily increased, almost to the limit of highest optical resolution. In this talk some new applications how they are used for Earth system observation purpose.

• International Journal of Automotive Technology
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• 제7권3호
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• pp.315-320
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• 2006

We have developed an active front steering system(AFS) with a planetary gear train, which can vary the steering gear ratio according to the vehicle speed and improve vehicle stability by superimposing steering angle. We conducted vehicle tests showing that co-operated control of AFS with ESP can improve vehicle stability by direct control of tire slip angle and that steering reaction torque during AFS intervention can be compensated by torque compensation using electric power steering.

• Journal of Advanced Marine Engineering and Technology
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• 제35권6호
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• pp.786-795
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• 2011

본 연구에서는 블레이드, 증속기, 발전기, 케이스를 포함한 풍력 발전시스템의 진동 모델을 개발 하였다. 특히 유성기어열에서의 유성기어는 유연핀에 지지가 되어 있는데, 이는 비틀림만을 고려하지 않고 유성기어의 회전 방향의 접선방향으로의 병진 운동을 고려하였으며, 풍력발전시스템이 마운트에 지지되어 있는 특징을 고려하여 케이스에 의한 운동을 포함 하였다. 풍력발전 시스템의 진동특성을 파악하기위하여, 풍하중, 불평형, 치합전달오차에 등에 의한 자려가진원을 구하였고, 운전속도 범위 내에서 위험속도 분석을 하였다. 위험속도해석결과, 2단 치통과 주파수에 의해서 81.2Hz, 104.7Hz 모드에서 공진이 발생하며, 3단 치통과 주파수에 의해서 264.5Hz, 377Hz, 424.6Hz 모드에서 공진이 발생하는 것을 알 수 있었다. 또한, 공진이 발생하는 진동모드를 분석하여 진동저감 대책을 수립하였다.

• 한국자동차공학회논문집
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• 제15권6호
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• pp.87-93
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• 2007

It is complicate to analysis the systems, dual mode hybrid systems, because they are composed of many planetary gear sets. For the performance test, it needs to define the systems with representative parameters. In this paper, system parameters, $\alpha$, $\beta$, $\zeta$, are introduced to define the systems, and an arbitrary system like E-IVT developed by Renault Motors is converted to the general system having equivalent parameters, such as $\beta'$, $R'_b$. Pontryagin principle and Kuhn-Tucker condition method are applied to solve the constrained problems, by which the methodology for accelerating test is generalized, and the results of the simulation are reported. In addition, the effects of alternative strategies are mentioned. The method of fuel economy test at engine mode is also introduced. The results of test at engine mode is different from the results of optimal trajectory, but the fuel economy of the engine mode is related to the highway driving and optimized operating of the system.

• 한국자동차공학회논문집
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• 제15권5호
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• pp.118-124
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• 2007

The efficiency of the hybrid systems which are composed of compound planetary gear sets depend on the amount of the recirculating energy among the motors and battery. This paper studies the analysis of the system efficiency with the parameters, ${\alpha},\;{\beta},\;{\gamma_a},\;{\gamma_b}$ and $\gamma_s$. The efficiency of the systems and the relative torque, speed and power of the power resources are represented by these parameters. The recuperating parameter $\kappa$ which makes the systems generalized is introduced, so the efficiencies of the modes such as the hybrid mode, the engine mode, the motoring mode and the recuperating mode are analyzed with simple equations. The tendency of the system efficiency according to the variations of the $\gamma_s$ and $\kappa$ are studied, by which it can be possible to reduce the loss of the power because the strategies for avoiding the singular speed ratio $\gamma_s$ are helpful for the system efficiency and specific value of $\kappa$ can increase the efficiency of the systems.

• Asian Journal of Atmospheric Environment
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• 제4권3호
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• pp.198-210
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• 2010

Precise analysis of local winds for the prediction of atmospheric phenomena in the planetary boundary layer is extremely important. In this study, wind profiler data with fine time resolution and density in the lower troposphere were used to improve the performance of a numerical atmospheric model of a complex coastal area. Three-dimensional variational data assimilation (3DVAR) was used to assimilate profiler data. Two experiments were conducted to determine the effects of the profiler data on model results. First, we performed an observing system experiment. Second, we implemented a sensitivity test of data assimilation intervals to extend the advantages of the profiler to data assimilation. The lowest errors were observed when using both radio sonde and profiler data to interpret vertical and surface observation data. The sensitivity to the assimilation interval differed according to the synoptic conditions when the focus was on the surface results. The sensitivity to the weak synoptic effect was much larger than to the strong synoptic effect. The hourly-assimilated case showed the lowest root mean square error (RMSE, 1.62 m/s) and highest index of agreement (IOA, 0.82) under weak synoptic conditions, whereas the statistics in the 1, 3, and 6 hourly-assimilated cases were similar under strong synoptic conditions. This indicates that the profiler data better represent complex local circulation in the model with high time and vertical resolution, particularly when the synoptic effect is weak.

• 한국인터넷방송통신학회논문지
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• 제19권2호
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• pp.243-253
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• 2019

행성 탐사의 첫 번째 단계는 일반적으로 자율적 탐사선을 사용하여 수행된다. 이 탐사선은 자신의 길을 찾고 행성표면에 대한 실험을 수행 할 수 있다. 이 논문에서는 각 에이전트의 지식과 노력을 공유하기 위해 블랙보드 시스템을 효과적으로 활용하는 다중 에이전트 시스템을 제안한다. 에이전트는 BDI (Belief Desire Intension) 모델의 조합으로 반응 모델을 사용하고 최단 거리를 계산하고 행성 표면에서 이동 경로를 계산하는 경로 찾기 알고리즘을 사용한다. 이 접근법은 짧은 시간 내에 주어진 지형에서 표면 탐사를 수행 할 수 있다. 블랙보드에 수집 된 정보는 상세한 표면 토양 변화 결과를 산출하는데 사용된다. 이 연구에서 제안된 다중 에이전트 시스템에 의한 탐사는 다양한 지형 크기별로 잘 수행되는 것으로 나타났다.

• 한국지리정보학회지
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• 제9권4호
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• pp.12-21
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• 2006

최근 우리는 항공 혹은 위성 영상 등에서 방대한 고해상도 지형 데이터를 접하고 있다. 여러 연구 및 응용에서 이러한 관심 지역의 대규모의 지리 정보 혹은 전체 행성 데이터에 대해서 실시간 시각화를 필요로 하고 있다. 널리 사용되고 있는 지형 실시간 시각화의 핵심적인 연산은 다중 상세도 수준 구조에서 참여자의 시점을 고려한 상세도 수준의 선택이다. 대규모 지리 데이터에 대해서 이러한 실시간 영상 생성을 수행하기 위해서는 실시간 영상 생성 시간 이전에 다계층 품질 계층구조를 구성하는 것이 필요하다. 본 연구에서는 전체 행성 응용을 위하여 정육면체 4-8 타일 구조를 선택하였다. 이를 기반으로, 원시 지형 정보 영역의 해당하는 단말 수준의 타일 구조를 선택적으로 구성하고, 생성된 타일에 대해서 샘플링을 통하여 단말 수준의 타일을 구성한다. 로우 패스 필터를 이용하여 상향식으로 저해상도 타일을 구성하여 전체 4-8 타일 다계층 구조를 완성한다. 본 연구는 비메모리 저장소에 4-8 타일 구조를 구성하기 위한 효과적인 일련의 방법론을 구체화하였으며, 공개되어 있는 전체 화성 지형 및 영상 데이터에 대해서 실험하였다.

• 천문학논총
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• 제27권4호
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• pp.181-182
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• 2012

Using the AKARI mid-infrared all-sky survey catalogue, we are searching for debris disks which are important objects as an observational clue to on-going planetary system formation. Debris disk candidates are selected through a significant excess of the measured flux over the predicted flux for the stellar photospheric emission at $18{\mu}m$. The fluxes were originally estimated based on the near-infrared spectral energy distributions (SEDs) of central stars constructed from the 2MASS J-, H-, and Ks-band fluxes. However, we found that in many cases the 2MASS photometry has large errors due to saturation in the central part of a star image. Therefore we performed follow-up observations with the IRSF 1.4m near-infrared telescope in South Africa to obtain accurate fluxes in the J-, H-, and Ks-bands. As a result, we have succeeded in improving the SEDs of the central stars. This improvement of the SEDs allows us to make more reliable selection of the candidates.

• International Journal of Aeronautical and Space Sciences
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• 제14권2호
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• pp.193-199
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• 2013

This work investigates the orbital perturbations of the cubesats that lie on LEO due to Earth albedo. The motivation for this paper originated in the investigation of the orbital perturbations for closed- Earth pico-satellites due to the sunlight reflected by the Earth (the albedo). Having assumed that the Sun lies on the equator, the albedo irradiance is calculated using a numerical model in which irradiance depends on the geographical latitude, longitude and altitude of the satellite. However, in the present work the longitude dependency is disregarded. Albedo force and acceleration components are formulated using a detailed model in a geocentric equatorial system in which the Earth is an oblate spheroid. Lagrange planetary equations in its Gaussian form are used to analyze the orbital changes when $e{\neq}0$ and $i{\neq}0$. Based on the Earth's reflectivity data measured by NASA Total Ozone Mapping Spectrometer (TOMS project), the orbital perturbations are calculated for some cubesats. The outcome of the numerical test shows that the albedo force has a significant contribution on the orbital perturbations of the pico-satellite which can affect the satellite life time.