• Journal of Mechanical Science and Technology
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• 제16권3호
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• pp.363-375
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• 2002

The effect of the electromagnetic force (or Lorentz force) on the flow behavior around a circular cylinder is investigated by computation. Two-dimensional unsteady flow computation for Re=10$^2$is carried out using a numerical method of finite difference approximation in a curvilinear body-fitted coordinate system by solving the momentum equations including the Lorentz force as a body force. The effect of spatial variations of the Lorentz forcing region and forcing direction along the cylinder circumference is investigated. The numerical results show that the Lorentz force can effectively suppress the flow separation and oscillation of the lift force of circular cylinder cross-flow, leading to reduction of drag.

• 한국마린엔지니어링학회:학술대회논문집
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• 한국마린엔지니어링학회 2006년도 전기학술대회논문집
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• pp.305-306
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• 2006

Developed in this study is a nonlinear Ekman pumping model to be used in simulating the rotating flows with quasi-three-dimensional Navier-Stokes equations. In this model, the Ekman pumping velocity is given from the solution of the Ekman boundary-layer equations for the region adjacent to the bottom wall of the flow domain; the boundary-layer equations are solved in the momentum-integral form. The developed model is then applied to rotating flows in a rectangular container receiving a time-periodic forcing. By comparing our results with the DNS and experimental data we have validated the developed model. We also compared our results with those given from the classical Ekman pumping model. It was found that our model can predict tile rotating flows more precisely than the classical linear model.

• 대한기계학회논문집B
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• 제30권6호
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• pp.568-577
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• 2006

Developed in this study is a nonlinear Ekman pumping model to be used in simulating the rotating flows with quasi-three-dimensional Navier-Stokes equations. In this model, the Ekman pumping velocity is given from the solution of the Ekman boundary-layer equations for the region adjacent to the bottom wall of the flow domain; the boundary-layer equations are solved in the momentum-integral form. The developed model is then applied to rotating flows in a rectangular container receiving a time-periodic forcing. By comparing our results with the DNS and experimental data we have validated the developed model. We also compared our results with those given from the classical Ekman pumping model. It was found that our model can predict the rotating flows more precisely than the classical linear model.

• 대기
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• 제26권3호
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• pp.401-412
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• 2016

A 3D sonic anemometer has been installed at Yongpyong alpine slope since Oct. 23th 2014 to observe the slope winds and to analyze turbulent characteristics with the change in surface cover (grass and snow) and the synoptic wind strength. Eddy covariance method has been applied to calculate the turbulent quantity after coordinate transformation of a planar-fit rotation. We have carefully selected 3 good episodes in the winter season (23 October 2014 to 28 February 2015) for each category (9 days in total), such as grass and snow covers in case of weak synoptic wind condition, and grass cover of strong synoptic wind. The diurnal variations of the slope winds were well developed like the upslope wind in the daytime and downslope wind in the nighttime for both surface covers (grass and snow) in the weak synoptic forcing, when accordingly both heat and momentum fluxes significantly increased in the daytime and decreased in the nighttime. Meanwhile, diurnal variation of heat flux was not present on the snow cover probably in associated with significant fraction of sunlight reflection due to high albedo especially during the daytime in comparison to those on the grass cover. In the strong synoptic regime, the most dominant feature at Yongpyong, only the southeasterly downslope winds were steadily generated irrespective of day and night with significant increases in momentum flux and turbulent kinetic energy as well, which could suggest that local circulations are suppressed by the synoptic scale forcing. In spite of only one season analysis applied to the limited domain, this kind of an observation-based study will provide the basis for understanding of the local wind circulation in the complex mountain domain such as Gangwon in Korea.

• Ocean and Polar Research
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• 제34권3호
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• pp.287-296
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• 2012

In the theory of source-driven abyssal circulation, the forcing is usually assumed to be steady source (deep-water formation). In many cases, however, the deep-water formation occurs instantaneously and it is not clear whether the theory can be applied well in this case. An attempt is made to resolve this problem by using a simple reduced gravity model. The model basin has large depth change compared for its size, like the East Sea, such that isobaths nearly coincide with geostrophic contours. Deep-water is formed every year impulsively and flows into the model basin through the boundary. It is found that the circulation driven by the impulsive source is generally the same as that driven by a steady source except that the former has a seasonal fluctuation associated with unsteadiness of forcing. The magnitudes of both the annual average and seasonal fluctuations increase with the rate of deep-water formation. The problem can be approximated to that of linear diffusion of momentum with boundary flux, which well demonstrates the essential feature of abyssal circulation spun-up by periodic impulsive source. Although the model greatly idealizes the real situation, it suggests that abyssal circulation can be driven by a periodic impulsive source in the East Sea.

• 한국가시화정보학회:학술대회논문집
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• 한국가시화정보학회 2007년도 추계학술대회
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• pp.134-137
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• 2007

The temporal evolution of wake behind a circular cylinder oscillating rotationally with a relatively high forcing frequency has been investigated experimentally using a dynamic PIV technique. Experiments were carried out with varying the frequency ratio $F_R\;(=f_f/f_n)$ in the range from 0.0 (stationary) to 1.6 at oscillation amplitude of ${\theta}_A=30^{\circ}$ and Reynolds number of $Re=4.14{\times}10^3$. Depending on the forcing condition ($F_R$), the flow was divided into three regimes; non-lock-on ($F_R=0.4$), transition ($F_R=0.8$, 1.6) and lock-on regimes ($F_R=1.0$) with markedly different flow structure in the near-wake region behind the cylinder. When the frequency ratio was less than 1.0 ($F_R{\le}1.0$), the rotational oscillatory motion of the cylinder decreased the length of the vortex formation region and enhanced the mutual interaction between large-scale vortices across the wake centerline. The entrainment of ambient fluid seemed to play an important role in controlling the near-wake flow and shear-layer instability. However, the flow characteristics changed markedly beyond the lock-on flow regime ($F_R=1.0$) due to high-frequency forcing. At $F_R=1.6$, the mutual interactions between the vortices shed from both sides of the cylinder were not so strong. Thereby, the flow entrainment and momentum transfer into the wake center region were reduced. In addition, the size of the large-scale vortices decreased since the lateral extent of the wake was suppressed.

• Journal of Astronomy and Space Sciences
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• 제22권2호
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• pp.147-174
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• 2005

본 연구에서는 미 국립대기연구소(NCAR)의 열권-이온권 전기역학적 대순환 모델(TIEGCM)을 이용하여 행성간 자기장(IMF)의 방향과 세기 그리고 고도에 따라 여름철 남반구 고위도 하부 열권의 바람에 작용하는 운동량 강제력을 정량적으로 구하였다. 그리고 이들을 서로 비교 분석함으로써 IMF 조건과 고도에 따른 고위도 하부 열권의 풍계(wind system)를 유지시켜주는 주된 물리적인 과정을 살펴보았다. 고위도 하부 열권(<180km)에서 양($B_y$ > 0.8|$\overline{B}_z$|)또는 음($B_y$ < -0.8|$\overline{B}_z$|)의 IMF By 조건인 경우에 운동량 강제력 차이, 즉 IMF 기준치 ${\neq}$ 0 일 때와 IMF 기준치=0 일 때의 운동량 강제력 차이(difference momentum force)는 자기위도 -80$^{\circ}$에서 최대값을 가지면서 극관과 오로라 영역에 국한된 단순한 형태의 분포를 보인다. 그리고 IMF $B_z$ 성분이 양과 음일 때 강제력 차이의 세기는 비슷하지만 분포양상은 반대방향을 취한다. 한편 IMF $B_z$가 양($B_z$ > 0.3125|$\overline{B}_y$|) 또는 음($B_z$ < -0.3125|$\overline{B}_y$|)인 조건인 경우에는 강제력 차이가 아오로라(subauroral) 위도까지 분포하며 IMF $B_z$가 양 또는 음의 조건일 때 보다 복잡한 구조를 보인다. 그리고 IMF $B_z$가 음인 경우의 강제력 차이가 양인 경우보다 더 크며 반대방향으로 작용한다. 125km 보다 더 높은 고도(>125km)에서 바람차이를 결정하는 주된 강제력은 기압경도력, 전향력, 수평이류 그리고 비발산 성분이 강한 Pedersen 이온항력인 것으로 확인되었다. 고도 약 125km 에서는 이 네 가지 힘에 더불어 비회전 성분이 강한 Hall 이온향력과 극관내 의 연직 이류가 지역과 시간에 따라 바람차이의 형성에 작용한다. 한편 고도 108-125km 에서는 IMF $B_z$ 조건일 경우의 극관영역을 제외하고는 기압경도력, 전향력 그리고 Hall 이온항력이 이 고도에서의 바람차이를 유발시키는 주된 강제력으로 작용한다. 고도 108km 이하에서는 기압경도력과 전향력이 균형을 이루어 지균 운동을 유지시킨다. IMF-$\overline{B}_y$의존 MLT 평균 운동량 강제력들은 이온항력을 제외한 다른 모든 남북성분이 동서성분에 비해 더 강하게 중성대기에 작용하는 것으로 확인되었다. 108-125km의 고도에서 IMF B?가 음인 경우에 이온항력은 하강운동 및 단열압축가열과 관련된 시계방향의 온난순환(warm circulation)을 극관 내에 형성시킨다. 반면 IMF $B_y$가 양인 경우에는 극관 내에 상승운동 및 단열팽창냉각과 관련된 반시계방향의 한랭순환(cold circulation)을 형성시킨다. 이온항력은 IMF $B_z$가 음인 경우에는 새벽영역에 상승운동과 관련된 반시계방향의 한랭순환을, 반면에 IMF $B_z$가 양인 경우에는 새벽영역에 하강운동과 관련된 시계방향의 온난순환을 형성시킨다.

• 한국해안·해양공학회논문집
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• 제24권6호
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• pp.390-399
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• 2012

본 연구에서는 지속적인 담수유입이 존재하고 S자의 수로형태를 가진 경기만 석모수로에서 소조기 홍수시 13시간 동안 7개의 정선에서 단면유속 및 염분을 관측하였다. 각 단면의 최강 창조와 낙조시의 유속 크기와 방향을 파악하였고, 단면 내의 유속 분포 및 염분구조를 분석하였다. 또한 정선 별로 나타나는 횡 방향 흐름이 어떠한 운동량에 의해 지배되는지 파악하고자 횡 방향의 운동량 분석을 수행하였다. 운동량 분석에서는 석모수로의 S자 형태의 영향을 고려하기 위해서 원심력을 고려하였다. 분석 결과 소조기 홍수시 석모수로는 횡 방향 압력 경도력과 수직적 마찰력이 가장 우세하기 때문에 염분 분포와 성층에 의한 흐름이 주로 나타났다. 수로의 특성은 크게 북단과 남단으로 나누어 볼 수 있는데 상대적으로 조간대가 넓게 형성되고 담수의 영향이 큰 석모수로 북단의 4개 정선중에서 수심이 깊은 정선에서는 횡 방향 압력 경도력이 우세하지만 수직적으로 크기가 다르며, 수심이 낮은 정선에서는 수직 마찰항이 우세하였다. 이와는 달리 수심이 깊고 수로의 굴곡이 심한 석모수로 남단에서는 낙조시 지형학적 원인과 담수의 영향에 따라 이류 가속항과 원심력이 강해지게 된다. 이와 같은 결과를 종합할 때, 석모수로는 위치와 수심, 수로의 굴곡 등에 따라 운동량 분포가 각기 달리 나타나며 이러한 영향으로 인해 횡 방향 흐름 특성이 발생했음을 알 수 있다.

• 대한기계학회:학술대회논문집
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• 대한기계학회 2000년도 춘계학술대회논문집B
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• pp.704-708
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• 2000

A new efficient numerical method for computing unsteady, incompressible flows, DRANS (Decoupled Reynolds-Averaged Navier-Stokes), is presented. To eliminate the restriction of CFL condition, a fully-implicit time advancement in which the Crank-Nicolson method is used fer both the diffusion and convection terms. is adopted. Based on decomposition method, the velocity-turbulent quantity decoupling is achieved. The additional decoupling of the intermediate velocity components in the convection term is made for the fully-implicit time advancement scheme. Since the iterative procedures for the momentum, ${\kappa}\;and\;{\varepsilon}$ equations are not required, the components decouplings bring fourth the reduction of computational cost. The second-order accuracy in time of the present numerical algorithm is ascertained by computing decaying vortices. The present decoupling method is applied to turbulent boundary layer with local forcing.

• 전기학회논문지
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• 제62권1호
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• pp.43-48
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• 2013

In this paper, magnetic buoyancy force on nonmagnetic solid object submerged in magnetic liquid was simulated and measured. For the evaluation of the force, a multi-physics approach of hydrostatic equilibrium considering magnetic body force as well as gravity is presented. The magnetic body force should be regarded as an additional forcing term in the momentum equation of hydrodynamics. It is also shown that the virtual air-gap based Kelvin's force formula is a useful method for the calculation of force distribution in the magnetic liquid. The experimental result which was performed by a load-cell measurement system agreed quantitatively well with the numerical one.