• 천문학회보
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• 제42권2호
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• pp.45.2-45.2
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• 2017

Using the latest cosmological hydrodynamic N-body simulations of groups and clusters, we study how location in phase-space coordinates at z = 0 can provide information on environmental effects acting in clusters. We confirm the results of previous authors showing that galaxies tend to follow a typical path in phase-space as they settle into the cluster potential. As such, different regions of phase-space can be associated with different times since first infalling into the cluster. However, in addition, we see a clear trend between total mass loss due to cluster tides and time since infall. Thus, we find location in phase-space provides information on both infall time and tidal mass loss. We find the predictive power of phase-space diagrams remains even when projected quantities are used (i.e.,line of sight velocities, and projected distances from the cluster). We provide figures that can be directly compared with observed samples of cluster galaxies and we also provide the data used to make them as supplementary data to encourage the use of phase-space diagrams as a tool to understand cluster environmental effects. We find that our results depend very weakly on galaxy mass or host mass, so the predictions in our phase-space diagrams can be applied to groups or clusters alike, or to galaxy populations from dwarfs up to giants.

• 한국해양공학회지
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• 제33권5호
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• pp.400-410
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• 2019

In this study, the numerical code for the 3D nonlinear dynamic analysis of an SLWR (Steel Lazy Wave Riser) was developed using the lumped mass line model in a FORTRAN environment. Because the lumped mass line model is an explicit method, there is no matrix operation. Thus, the numerical algorithm is simple and fast. In the lumped mass line model, the equations of motion for the riser were derived by applying the various forces acting on each node of the line. The applied forces at the node of the riser consisted of the tension, shear force due to the bending moment, gravitational force, buoyancy force, riser/ground contact force, and hydrodynamic force based on the Morison equation. Time integration was carried out using a Runge-Kutta fourth-order method, which is known to be stable and accurate. To validate the accuracy of the developed numerical code, simulations using the commercial software OrcaFlex were carried out simultaneously and compared with the results of the developed numerical code. To understand the nonlinear dynamic characteristics of an SLWR, dynamic simulations of SLWRs excited at the hang-off point and of SLWRs in regular waves were carried out. From the results of these dynamic simulations, the displacements at the maximum bending moments at important points of the design, like the hang-off point, sagging point, hogging points, and touch-down point, were observed and analyzed.

• 한국해양환경ㆍ에너지학회지
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• 제14권2호
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• pp.107-113
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• 2011

해수유동모델의 검증 및 평가를 위해 적용되는 또는 적용가능한 10종류의 모델 오차평가방법 - 네가지의 정량적 평가방법(절대평균오차, 평균제곱근 오차, 상대적 절대평균오차, 백분율모델오차)과 여섯가지의 정성적 평가방법(상관계수, 신뢰지수, 일치지수, 모델효율성, 비용함수, 잔여량계수) - 을 소개하고, 실제 조위, 유속, 염분관측치와 3차원 곡선형 모델(CH3D)에서 구해진 플로리다 하구에서의 수치해에 이들 모델 오차평가방법들을 적용하였다. 조위 및 유속평가시 절대평균오차, 평균제곱근 오차, 상대적 절대평균오차, 상관계수, 일치지수, 모델효율성, 비용함수, 잔여량계수 등이 적합하였다. 그리고 염분평가시 절대평균오차, 평균제곱근 오차, 상대적 절대평균오차, 백분율모델오차, 상관계수, 신뢰지수, 비용함수, 잔여량계수 등의 사용이 타당하였다. 정량/정성적 평가방법들이 서로 유사한 평가경향을 보여 줌으로써, 상호간의 신뢰성도 보여 주었다. 다양한 모델 오차평가방법을 통하여 계산된 평가값을 토대로, 본 연구에서는 조위, 유속, 염분이 잘 재현된 해수유동모델의 평가범위를 제시하였다. 조위의 경우 상대적 절대평균 오차는 10%이내, 상관계수는 0.95이상, 일치지수는 0.98이상, 모델효율성은 0.93이상, 비용함수는 0.21이내이며, 유속의 경우 상대적 절대평균오차는 20%이내, 상관계수는 0.7이상, 일치지수는 0.8이상, 모델효율성은 0.5이상, 비용 함수는 0.5이내이며, 염분의 경우 상대적 절대평균오차와 백분율모델오차는 10%이내, 상관계수는 0.9이상, 신뢰지수는 1.15이내, 비용함수는 0.1이내 이다.

• 수산해양기술연구
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• 제38권2호
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• pp.164-171
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• 2002

본 연구에서는 중층 트롤 어구 시스템의 운동을 예측하기 위한 운동방정식을 정의하였고 중층 트롤 어구 시스템의 운동을 유체역학적으로 해석하여 시뮬레이션에 적용하여 계산한 결과를 해상에서 실험한 결과들과 비교하여 시뮬레이션의 정확도를 검증하였다. 해상실험은 1997년 8월 28일부터 1997년 8월 30일까지 동해상(36$^{\circ}$05'N, 130$^{\circ}$25'2E~36$^{\circ}$20'N,130$^{\circ}$47'E)에서 부경대 실습선 가야호를 이용하여 실시하였다. 그 결과는 다음과 같다. 1. 중층 트롤 시스템의 운동을 해석하기 위해 사용된 운동 방정식은 m$_{i}$equation omitted/=f$_{i}$으로 기술하였고, 여기서 m과 /equation omitted/는 각각 질점 i의 질량과 가속도이며, f$_{i}$는 질점에 작용하는 힘이다. 2. 각 질점에 작용하는 힘은 내력과 외력으로 구성되며, 내력은 질점 사이에서 작용하는 힘으로 어구 시스템 구성에 사용된 각 종 줄과 그물실의 탄성에 의한 힘이며, 외력은 질점에 작용하는 저항, 부력 그리고 중력 등이다. 3. 시뮬레이션의 결과를 해상실험의 결과와 정량적으로 비교하기 위해 끌줄길이 250m, 예망속력 2m/s에서의 전개판 간격, 전개판 수심 망고 그리고 망폭을 비교하였다. 이 때 전개판 사이의 간격과 망폭은 계산치와 실험치가 거의 일치하며, 전개판의 수심과 망고는 각각 5m와 4m의 오차를 가지고 있었다. 4. 시뮬레이션 도중 끌줄의 길이, 예망속력, 부력 그리고 전개판 면적을 증가시키면서 어구의 형상을 계산한 결과를 앞선 해상 실험들의 결과와 비교하였다. 이 때 끌줄길이를 증가시킨 경우 어구의 예망수심이 깊어졌으며 전개판의 간격이 증가하였다. 예망속력을 증가시킨 경우 어구가 수면으로 부상하였으며 전개판의 간격이 줄어들었다. 부력을 증가시킨 경우에도 어구가 수면으로 부상하였으며 전개판의 간격과 망폭이 줄어들었다. 마지막으로 전개판의 면적을 증가시킨 경우에는 전개판의 전개력이 증가하여 전개판 사이 간격이 커지고 망폭이 증가하였다.

• 대한조선학회논문집
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• 제50권1호
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• pp.1-7
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• 2013

The high-skewed and/or composite propellers of current interests to reduce the ship vibration and to increase the acoustic performance are likely to be exposed to the unexpected structural problems. One typical example is that the added mass effect on the propellers working in the non-uniform wake field reduces the natural frequency of the propeller leading to the resonance with the low-frequency excitation of the external forces. To avoid this resonance problem during the design stage, the technique of fluid-structure interaction has been developed, but the higher-order effect of the blade geometry deformation is not yet considered in evaluating the added mass effects. In this paper the fluid boundary-value problem is formulated by the potential-based panel method in the inviscid fluid region with the velocity inflow due to the body deformation, and the structural response of the solid body under the hydrodynamic loading is solved by applying the finite element method which implements the 20-node iso-parametric element model. The fluid-structure problem is solved iteratively. A basic fluid-sturcture interaction study is performed with the simple rectangular plates of thin thickness with various planform submerged in the water of infinite extent. The computations show good correlation with the experimental results of Linholm, et al. (1965).

• 천문학회보
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• 제40권2호
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• pp.34.2-34.2
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• 2015

We aim to investigate the formation of primordial globular clusters (GCs) in the isolated dwarf galaxy (${\sim}10^{10}M_{sun}$) with cosmological zoom-in simulations. For this, we modified cosmological hydrodynamic code, GADGET-3, in a way to include the radiative heating/cooling that enables gas particles cool down to T~10K, reionization (z < 8.9) of the Universe, UV shielding ($n_{shield}$ > $0.014cm^{-3}$), and star formation. Our simulation starts in a cubic box of a side length 1Mpc/h with 17 million particles from z = 49. The mass of each dark matter (DM) and gas particle is $M_{DM}=4.1{\times}10^3M_{sun}$ and $M_{gas}=7.9{\times}10^2M_{sun}$, respectively, thus the GC candidates can be resolved with more than hundreds particles. We found the following results: 1) mini halos with the more interactions before merging into the main halo form the more stars and thus have the higher star mass fraction ($M_{star}/M_{total}$), 2) the mini halos with the high $M_{star}/M_{total}$ can survive longer and thus spiral into closer to the galactic center, 3) the majority of them spiral into bulge, but some of them can survive until the last as baryon-dominated system, like the GC.

• 상하수도학회지
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• 제31권6호
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• pp.481-490
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• 2017

Water and wastewater treatment has always been a challenging task due to the continuous increase in amount and the change in characteristics of the poorly biodegradable and highly colored organic matters, as well as harmful micro-organisms. Advanced techniques are therefore required to successfully remove these pollutants from water before reuse or discharge to receiving water bodies. Application of ozone, which is a powerful oxidant and disinfectant, alone or as part of advanced oxidation process depends on the complex kinetic reactions and the mass transfer of ozone involved. Micro- and nano bubbling considerably improves gas dissolution compared to conventional bubbles and hence mass transfer. It can also intensify generation of hydroxyl radical due to collapse of the bubbles, which in turn facilitates oxidation reaction under both alkaline as well as acidic conditions. This review gives the overview of application of micro- and nano bubble ozonation for purification of water and wastewater. The drawbacks of previously considered techniques and the application of the hydrodynamic ozonation to synthetic aqueous solutions and various industrial wastewaters are systematically reviewed.

• 한국소음진동공학회:학술대회논문집
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• 한국소음진동공학회 2008년도 춘계학술대회논문집
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• pp.96-100
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• 2008

In this paper, a experimental and theoretical study is carried out on the hydroelastic vibration for a rectangular bottom and side plate of tank. It is assumed that the tank wall is clamped along the plate edges. The fluid velocity potential is used for the simulation of fluid domain and to obtain the added mass due to plate vibration. It is assumed that the fluid is imcompressible and inviscid. Assumed mode method is utilized to the plate model and hydrodynamic force is obtained by the proposed approach. The coupled natural frequencies are obtained from the relationship between kinetic energies of a wall including fluid and the potential energy of the wall. The theoretical result is compared with the three-dimensional finite element method. In order to verify the result, modal test was carried out for bottom/side plate of tank model by using impact hammer. It was found the fundamental natural frequency of bottom plate is lower than that of side plate of tank and theoretical result was in good agreement with that of commercial three-dimensional finite element program.

• 천문학회보
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• 제42권1호
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• pp.38.1-38.1
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• 2017

We report the results of three-dimensional radiation hydrodynamic simulations of star cluster formation in turbulent molecular clouds, with primary attention to how stellar radiation feedback controls the lifetime and net star formation efficiency (SFE) of their natal clouds. We examine the combined effects of photoionization and radiation pressure for a wide range of cloud masses (10^4 - 10^6 Msun) and radii (2 - 80 pc). In all simulations, stars form in densest regions of filaments until feedback becomes strong enough to clear the remaining gas out of the system. We find that the SFE is primarily a function of the initial cloud surface density, Sigma, (SFE increasing from ~7% to ~50% as Sigma increases from ~30 Msun/pc^2 to ~10^3 Msun/pc^2), with weak dependence on the initial cloud mass. Control runs with the same initial conditions but without either radiation pressure or photoionization show that photoionization is the dominant feedback mechanism for clouds typical in normal disk galaxies, while they are equally important for more dense, compact clouds. For low-Sigma clouds, more than 80% of the initial cloud mass is lost by photoevaporation flows off the surface of dense clumps. The cloud becomes unbound within ~0.5-2.5 initial free-fall times after the first star-formation event, implying that cloud dispersal is rapid once massive star formation takes place. We briefly discuss implications and limitations of our work in relation to observations.

• 한국전산유체공학회:학술대회논문집
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• 한국전산유체공학회 2008년도 춘계학술대회논문집
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• pp.21-24
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• 2008

The present study numerically investigates the glottal airflow characteristics as well as acoustic features of phonation fully coupled with dynamic behavior of vocal folds. The vocal folds are described by a low-dimensional body-covered model characterized by bio-mechanical parameters such as glottal width, vocal folds stiffness, and subglottal pressure. The flow in the vocal tract is modeled as an incompressible, axisymmetric form of the Navier-Stokes equations (INS), while the acoustic field is predicted by the linearized perturbed compressible equations (LPCE). The computed result shows that a two-mass model of vocal folds is sufficient to reproduce temporal variations in oral airflow and glottis motion produced by female speakers. It is also found that i) the glottal width has a significant effect on the amplitude of glottal flow, and thus on the amplitude of acoustic wave in the vocal tract, ii) the vocal fold tension is the main control parameter for the fundamental frequency of phonation, iii) the subglottal pressure plays an appreciable role on reproduction of the self-sustained oscillation of vocal folds, and iv) the strength of pulsating airflow and vortical structures are primarily affected by glottal width and subglottal pressure, and are closely related to pitch, loudness, and voice quality. Finally, more comprehensive explanation about the difference between one- and two-mass models is presented with discussion of effectiveness of vocal folds oscillation and voice quality.