• 한국정밀공학회지
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• 제17권6호
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• pp.111-118
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• 2000

The design of reference trajectory with respect to drag acceleration is necessary to decelerate from hypersonic speed safely after atmosphere re-entry of space vehicle. The re-entry guidance design involves trajectory optimization, generation of a reference drag acceleration profile with the satisfaction of 6 trajectory constraints during the re-entry flight. This reference drag acceleration profile can be considered as the reference trajectory. The cost function is composed of the accumulated total heating on vehicle due to the reduction of weight. And a regularization is needed to prevent optimal drag profile from varying too fast and achieve realized trajectory. This paper shows the relations between velocity, drag acceleration and altitude in drag acceleration profile, and how to determine the reference trajectory.

• 동력기계공학회지
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• 제7권4호
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• pp.67-73
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• 2003

The entry guidance design involves trajectory optimization and generation of a drag acceleration profile as the satisfaction of trajectory conditions during the entry flight. The reference trajectory is parameterized and optimized as piecewise linear functions of the velocity. A regularization technique is employed to achieve desired properties of the optimal drag profile. The regularized problem has smoothness properties and the minimization of performance index then prevents the drag acceleration from varying too fast, thus eliminating discontinuities. This paper shows the trajectory control using the simple control law as well as the information of reference drag acceleration.

• 한국마린엔지니어링학회:학술대회논문집
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• 한국마린엔지니어링학회 2001년도 추계학술대회 논문집(Proceeding of the KOSME 2001 Autumn Annual Meeting)
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• pp.130-134
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• 2001

In the re-entry control system, errors apt to induce because the time derivative of drag acceleration is analytically estimated. Still more, the difficulty of estimation of the exact drag coefficient in hypersonic velocity and the nun-reality of the scale height cause a steady-state drag error. This paper proposes the additional method of the disturbance observer. This reduces the steady-state drag error according to the following series. First, this method estimates a error in drag acceleration time derivative by the analytic calculation and then creates the new drag acceleration time derivative using the estimated error. The performance of the re-entry control system is verified about 32 reference trajectories.

• 한국정밀공학회:학술대회논문집
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• 한국정밀공학회 1997년도 추계학술대회 논문집
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• pp.361-364
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• 1997

The re-enty guidance design involves trajectory optimization, generation of a reference drag acceleration profile with the satisfaction of trajectory constraints. This reference drag acceleration profile can be considered as the reference trajectory. This paper proposes the atmospheric re-entry system which is composed of longitudinal, later and range control. This paper shows the a performance of a re-entry guidance and control system using feedback linearization control and predictive control.

• 대한조선학회논문집
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• 제56권6호
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• pp.507-514
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• 2019

Computational studies of accelerating flow around 2D Circular Cylinder was performed to investigate characteristics of wake field and drag forces. Previous studies had revealed that drag on the cylindrical body in accelerating flow is much greater than that in the flow with constant velocity; however, the underlying physics on the drag increase has not been clearly investigated. In order to investigate the drag increase and its relationship with wake development, this study employed a finite-volume based CFD code, Fluent 13.0 with k-ω SST model for turbulence effects. Inflows are modeled with varied accelerations from 0.4905 to 9.81m/s². The drag computed in the present study is in good agreement with previous studies, and clearly shows the increase compared to the drag on the body in the flow with constant velocity. The results also show that drag crisis observed at high Reynolds number in the case of the flow with constant velocity is also found in the case of accelerating flow. The analysis for wake and recirculation length shows that conventional vortex shedding does not occur even at high Reynolds number and the drag increase is larger at higher acceleration.

• 한국전산유체공학회:학술대회논문집
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• 한국전산유체공학회 2010년 춘계학술대회논문집
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• pp.214-220
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• 2010

This article described that a high Reynolds number version of a turbulence model was modified by using drag reduction to analyze the turbulent flows of non-Newtonian fluid with visco-elastic viscosity and it was applied hemodynamics which was representative of visco-elastic fluid. The turbulence characteristics of visco-elastic fluid was expanded viscous sublayer region and buffer layer region by drag reduction phenomenon and also Newtonian turbulence models does not predict because viscosity was related with shear rate of fluid flow. Hence numerical simulation using a modified turbulence model was conducted under the same conditions that were applied to obtain the experiment results and previous turbulence models and then the numerical investigation of turbulent blood flow in the stenosed artery bifurcation under periodic acceleration of the human body.

• Journal of Astronomy and Space Sciences
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• 제24권2호
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• pp.125-134
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• 2007

이 연구에서는 태양 및 지자기 활동에 의해 발생한 우주환경변화가 우리나라 위성인 아리랑위성1호(KOMPSAT-1)의 궤도에 미치는 영향을 분석하였다. 인공위성의 궤도변화는 정상적인 상태에서도 자연적인 섭동에 의해 지속적으로 발생하지만, 거대한 태양폭발에 의한 지구 주변 우주환경이 급격히 변화할 때 고층대기의 밀도변화로 인해 크게 발생한다. 특히 이러한 현상은 아리랑위성 1호와 같이 저궤도 상에서 운영되는 위성에 직접적인 영향을 미친다. 이 때, 태양활동에 의한 지구 주변 우주환경의 변화는 크게 두 가지로 구분할 수 있다. 하나는 태양 플레어 (Flare)가 폭발했을 때 고에너지 복사(Radiation)로 인해 지구 고층대기가 가열되어 팽창하고 이런 결과로 고층대기에 있는 중성입자밀도가 급격히 증가하는 것이다. 다른 하나는 코로나 물질 방출(Coronal Mass Ejections) 등에 의해 발생한 지자기폭풍기간 동안 플라즈마 대류와 입자들의 하강으로 전기장이 강해져 상당량의 줄가열(Joule heating)과 하강입자가열(precipitating particle heating)이 발생하고 이로 인해 중성입자밀도가 증가하는 것이다. 두 가지 원인에 대한 영향을 구분하여 알아보기 위해, 우리는 태양 및 지자기 자료를 면밀히 분석하여 2001년에서 2002년 동안 5개의 기간을 선정하였다. 그 결과 위성의 대기저항가속도는 태양의 극자외선(Extreme Ultra-Violet)의 증가와 함께 약 하루 정도의 시간 지연을 가지고 유사하게 변화하고 있음을 확인하였다(R=0.92). 그리고 지자기폭풍이 발생한 기간동안 대기저항가속도는 지자기폭풍에 의한 Dst 변화와 상당히 유사하게 그리고 거의 동시에 급격히 변화하는 것을 확인하였다. 마지막으로 우리는 위성의 대기저항가속도의 변화는 전반적으로는 오랜 기간 동안 고에너지 복사에 의한 효과로 나타나고 있으나 짧은 기간(하루 미만) 동안 크게 발생하는 대기저항가속도의 변화는 지자기폭풍에 의한 효과로 보고 있다.

• Tribology and Lubricants
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• 제35권2호
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• pp.123-131
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• 2019

This study characterizes the coastdown performances of two small electric motors supported on high-speed ball bearings (BBs) and gas foil bearings (GFBs), and it predicts their acceleration performances. The two motors have identical permanent magnetic rotors and mating stators. However, the shaft of the GFBs has a larger mass and polar/transverse moments of inertia than that of the BBs. Motor coastdown tests demonstrate that the rotor speed decreases linearly with the BBs and nonlinearly with the GFBs. A simple model for the BBs predicts a constant drag torque and linear decay of speed with time. The test data validate the model predictions. For the GFBs, the hydrodynamic lubrication model predictions reveal that the drag torque increases linearly with speed, and the speed decreases exponentially with time. The predictions agree very well with the test data in the speed range of 100-30 krpm. The boundary lubrication model predicts a constant drag torque and linear decay of speed with time. The predictions agree well with the test data below 15 krpm. Mixed lubrication occurs in the speed range of 30-15 krpm. Rotor acceleration performances are predicted based on the characteristics of deceleration performances. The GFBs require more time to reach 100,000 krpm than the BBs because of their larger shaft polar moment of inertia. However, predictions for the assumed identical polar moment of inertia reveal that the GFBs have a nearly identical acceleration performance to that of the BBs with a motor torque greater than $0.03N{\cdot}m$.

• 한국항공우주학회지
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• 제30권1호
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• pp.75-81
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• 2002

재진입 제어계에서는 항력가속도의 시간미분을 해석적으로 추정하므로 오차가 발생되기 쉽다. 더구나, 극초음속 영역에서의 정확한 항력계수 추정의 어려움과 스케일 고도의 비현실성도 정상상태오차의 원인이 된다. 우주왕복선의 경우, 제어계에 항력가속도 오차의 적분항을 첨가함으로서 정상상태 오차를 줄이는 방법을 취하였지만 페루프 시스템에 다극점을 갖게 하여 현대적인 제어기 합성에 어려움을 가져다 준다. 그러므로, 본 논문에서는 해석적 계산에 의해서 항력가속도 시간미분에 포함된 오차를 추정하고, 그 추정오차를 이용해 항력가속도 시간미분을 보정함으로써 정상상태 오차를 줄이는 방법인 외란 관측기의 설계를 제안하고자 한다. 결과로는 32개의 기준궤적을 대상으로 대기권 재진입 시스템의 성능을 검증해 본다.

• 한국우주과학회:학술대회논문집(한국우주과학회보)
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• 한국우주과학회 2004년도 한국우주과학회보 제13권2호
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• pp.278-280
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• 2004

GPS Navigation Solutions are used for operational orbit determination for the KOMPSAT-1 spacecraft. GPS point position data are definitely affected by systematic errors as well as noise. Indeed, the systematic error effects tend to be longer term since the GPS spacecrafts have periods of 12 hours. And then, the overlap method of determining orbit accuracy is always optimistic because of the presence of systematic errors with longer term effects. In this paper, we investigated the measurement noise and the system error for the KOMPSAT-l GPS Navigation Solutions. To assess orbit accuracy with this type of data, we use longer data arcs such as 5-7 days instead of 30 hour data arc. For this assessment, we should require much more attention to drag and solar radiation drag parameters or even general acceleration parameters in order to assess orbit accuracy with longer data arcs. Thus, the effects of the consideration of the drag, solar radiation drag, and general acceleration parameters were also investigated.