• 한국항행학회논문지
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• 제14권5호
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• pp.610-617
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• 2010

본 논문에서는 GPS 위성의 방송 궤도력 이상의 특성에 관하여 위성의 위치오차와 위성과 수신기 간 거리오차의 비교를 통해 분석하였다. 방송 궤도력 이상이 수신기의 위치 추정치에 미치는 영향은 위치오차에 의해 유발되는 거리오차와 밀접한 관련을 갖는다. 또한 거리오차는 위성 위치오차의 방향과 시선각 벡터의 방향에 의해 결정된다. 따라서 방송 궤도력 이상의 특성을 분석하기 위하여 방송 궤도력 각 변수를 위성 궤도의 크기와 모양을 결정하는 변수, 위성 궤도의 기울기를 결정하는 변수, 궤도에서의 위성의 위치를 결정하는 변수들로 분류하였다. 분류된 변수들의 특징을 바탕으로 위치변화가 수신기 위치 추정치에 미치는 영향을 분석하였다.

• 항공우주시스템공학회지
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• 제8권3호
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• pp.6-13
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• 2014

A passive launch and on-orbit vibration isolator using SMA(Shape Memory Alloy) washer for both the structural safety of the micro-vibration source by attenuating the transmitted force under launch loads and the micro-vibration isolation during their on-orbit operation has been proposed, which does not require the additional launch locking mechanism. To measure the characteristics of SMA mesh washer, we performed compressive loading tests with a single SMA mesh washer and a vibration isolator using SMA mesh washer. The numerical equivalent model of vibration isolator using SMA mesh washer composed of two spring and viscous damping elements has been verified that both stiffness and viscous damping varied with respect to compressed deformations. In addition, the effectiveness of launch loads and micro-vibration reduction has been investigated through the dynamic characteristics measurement test of cooler assembly combined with passive vibration isolator.

• International Journal of Aeronautical and Space Sciences
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• 제13권4호
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• pp.484-490
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• 2012

This paper is devoted to investigate the feasibility of using a medium power ground-based laser to produce a torque on LEO satellites of various shapes. The laser intensity delivered to a satellite is calculated using a simple model of laser propagation in which a standard atmospheric condition and linear atmospheric interaction mechanism is assumed. The laser force is formulated using a geocentric equatorial system in which the Earth is an oblate spheroid. The torque is formulated for a cylindrical satellite, spherical satellites and for satellites of complex shape. The torque algorithm is implemented for some sun synchronous low Earth orbit cubesats. Based on satellites perigee height, the results demonstrate that laser torque affecting on a cubesat has a maximum value in the order of $10^{-9}$ which is comparable with that of solar radiation. However, it has a minimum value in the order of $10^{-10}$ which is comparable with that of gravity gradient. Moreover, the results clarify the dependency of the laser torque on the orbital eccentricity. As the orbit becomes more circular it will experience less torque. So, we can conclude that the ground based laser torque has a significant contribution on the low Earth orbit cubesats. It can be adjusted to obtain the required control torque and it can be used as an active attitude control system for cubesats.

• 천문학회보
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• 제37권1호
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• pp.38.2-38.2
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• 2012

We use two-dimensional high-resolution MHD simulations to investigate the effects of magnetic fields on the formation and evolution of such substructures as well as on the mass inflow rates to the galaxy center. We find that there exists an outermost x1-orbit relative to which gaseous responses to an imposed stellar bar potential are completely different between inside and outside. Inside this orbit, gas is shocked into dust lanes and infalls to form a nuclear ring. Magnetic fields are compressed in dust lanes, reducing their peak density. Magnetic stress removes further angular momentum of the gas at the shocks and leads to a smaller and more centrally distributed ring, resulting in the mass inflow rates larger, by more than two orders of magnitude, than in the unmagnetized counterparts. Outside the outermost x1-orbit, on the other hand, an MHD dynamo operates near the corotation and bar-end regions, efficiently amplifying magnetic fields. The amplified fields shape into trailing magnetic arms with strong fields and low density. The base of the magnetic arms have a thin layer in which magnetic fields with opposite polarity reconnect via a tearing-mode instability. This produces numerous magnetic islands with large density which propagate along the arms to turn the outer disk into a highly chaotic state.

• Nuclear Engineering and Technology
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• 제38권1호
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• pp.69-80
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• 2006

Fluid-elastic instability in an air-water two-phase cross-flow has been experimentally investigated using two different arrays of straight tube bundles: normal square (NS) array and rotated square (RS) array tube bundles with the same pitch-to-diameter ratio of 1.633. Experiments have been performed over wide ranges of mass flux and void fraction. The quantitative tube vibration displacement was measured using a pair of strain gages and the detailed orbit of the tube motion was analyzed from high-speed video recordings. The present study provides the flow pattern, detailed tube vibration response, damping ratio, hydrodynamic mass, and the fluid-elastic instability for each tube bundle. Tube vibration characteristics of the RS array tube bundle in the two-phase flow condition were quite different from those of the NS array tube bundle with respect to the vortex shedding induced vibration and the shape of the oval orbit of the tube motion at the fluid-elastic instability as well as the fluid-elastic instability constant.

• Journal of Astronomy and Space Sciences
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• 제5권1호
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• pp.19-30
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• 1988

지구-달계의 질량비인 $\mu$-0.9878449 와 Jacobi 상수 2.9~3.4인 범위의 조건일 때 j종족 충돌궤도가 존재하는가를 조사하였다. 수치적인 방법으로는 Birckhoff의 정칙화 평면에서 Fehlberg(1968)의 5차 Runge-Kutta가변구간 수치적분방법을 사용하여 궤도의 주기성을 검증하였다. 그 결과 4개의 j종족 충돌궤도와 5개의 특이형궤도를 얻었고, 또한, 이 j 종족 충돌궤도가 Pinotsis와 Zikides(1984)가 제시한 주기와 궤도형태의 상관관계를 보였다.

• 한국정밀공학회:학술대회논문집
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• 한국정밀공학회 1995년도 춘계학술대회 논문집
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• pp.637-642
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• 1995

For measuring the error motion of ultra-precision spindle, eliminating the geometric errors is a must. Unless it is achieved, geometric errors will be dominant in data. Here, the roundness error and alignment error between spindle and sensor are to be removed. That's because typical error range of such spindle is muchless than geometric one. A capacitive transducer of cylidricalshape was developed, which takes full advantage of the spatial-averaging effect by using large area compared tpo the geometric error. This idea was first proposed by Chapman and here it is modified for better performance with nomical gap of 50 .mu. m and with newly designed guards which encompass the respective sensor to rectify the electrical field distribution in good shape. The measurement system is made to get the orbit of Ultra-Precision Air Spindle which is supposed to have its runout under 1 .mu. m. The Calibration data of this sensor is presented and the spindle orbit from 2000rpm to 5500rpm is showed. It is quite reasonable to use this sensor in the range of 60 .mu. m with an accuracy of several tens of nm.

• Advances in aircraft and spacecraft science
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• 제2권1호
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• pp.95-108
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• 2015

Automatic Dependent Surveillance Broadcast (ADS-B) is quickly being adopted by aviation safety authorities around the world as the standard for aircraft tracking. The technology provides the opportunity for live tracking of aircraft positions within range of an ADS-B receiver stations. Currently these receiver stations are bound by land and local infrastructural constraints. As such there is little to no coverage over oceans and poles, over which many commercial flights routinely travel. A low cost space based ADS-B receiving system is proposed as a constellation of small satellites. The possibility for a link between aircraft and satellite is dependent primarily on proximity. Calculating the likelihood of a link between two moving targets when considering with the non-periodic and non-uniform nature of actual aircraft flight-paths is non-trivial. This analysis of the link likelihood and the performance of the tracking ability of the satellite constellation has been carried out by a direct simulation of satellites and aircraft. Parameters defining the constellation (satellite numbers, orbit size and shape, orbit configuration) were varied between reasonable limits. The recent MH370 disappearance was simulated and potential tracking and coverage was analysed using an example constellation. The trend of more satellites at a higher altitude inclined at 60 degrees was found to be the optimal solution.

• 항공우주시스템공학회지
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• 제16권5호
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• pp.8-16
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• 2022

이 논문에서는 전천후 한반도 주변 감시를 위한 초소형 합성 개구 레이더 (synthetic aperture radar, SAR) 위성군의 배치를 위한 궤도 제어를 분석한다. 국내에서 개발하고 있는 Small SAR technology experimental project (S-STEP)는 한반도 주변 지역의 평균 재방문 주기를 확보하기 위해 여러 기의 위성이 여러 궤도 평면에 등간격으로 배치한다. 동일한 궤도 평면에 진입하는 여러 기의 위성들은 궤도 상에 등간격으로 분포하기 위해 발사체로부터의 분리 속도와 이온 추력기를 이용하여 궤도를 제어한다. 동일한 궤도 평면 상에 등간격으로 위성을 배치하는 궤도 전개를 위해 순간 추력으로 위성 사이의 표류율 차이를 조절해 위성군의 형상을 형성한다. 이 논문에서는 여러 가지 형태의 위성군을 제시하고 발사 전략에 따른 위성군의 배치 결과를 제시한다. 또한, 위성군을 형성하는 기간을 단축시키는 방법과 한계를 제시한다.

• 한국자기학회:학술대회 개요집
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• 한국자기학회 2014년도 자성 및 자성재료 국제학술대회
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• pp.98-99
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• 2014