• 제목/요약/키워드: Potential vorticity

검색결과 57건 처리시간 0.023초

문풀을 가지는 2차원 부유체의 강제 상하동요에 대한 CFD 해석 (CFD Analysis of Two-Dimensional Floating Body with Moon Pool under Forced Heave Motion)

  • 허재경;박종천
    • 한국해양공학회지
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    • 제25권2호
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    • pp.36-46
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    • 2011
  • A two-dimensional floating body with a moon pool under forced heave motion, including a piston mode, is numerically simulated. A dynamic CFD simulation is carried out to thoroughly investigate the flow field around a two-dimensional moon pool over various heaving frequencies. The numerical results are compared with experimental results and a linear potential program by Faltinsen et al. (2007). The effects of vortex shedding and viscosity are investigated by changing the corner shapes of the floating body and solving the Euler equation, respectively. The flow fields, including the velocity, vorticity, and pressure fields, are discussed to understand and determine the mechanisms of wave elevation, damping, and sway force.

병진운동하는 평판의 모서리에서의 3차원 와류 구조 가시화 (Three-dimensional vortex structure near a corner of a translating plate)

  • 김대겸
    • 한국가시화정보학회지
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    • 제13권1호
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    • pp.21-25
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    • 2015
  • Three-dimensional vortex structures in the corner region of translating normal plates are visualized experimentally with defocusing digital particle image velocimetry. Vortex formation processes for three plates with corner angle $60^{\circ}$, $90^{\circ}$, and $120^{\circ}$ are compared in order to study the effect of corner shape on vortex formation. In all cases, the self-induction of the starting vortex and its interaction with the potential flow induced by the moving plate cause the vortex to change its form dynamically after the plate starts to translate. While the vortex near a corner follows the plate in the low corner angle of $60^{\circ}$, the vortex separates early from the plate and its forward motion becomes slow in the high corner angle of $120^{\circ}$. It is also found that the starting vortex can transport inward at the corner, which depends on the corner angle.

Optimal Design of Two-Dimensional Cascade with Shock-Free Inflow Criterion

  • Muis, Abdul;Sutikno, Priyono;Soewono, Aryadi;Hartono, Firman
    • International Journal of Fluid Machinery and Systems
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    • 제9권4호
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    • pp.362-369
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    • 2016
  • The shock-free inflow criterion applied in the development of two-dimensional cascade for turbomachinery design. The developed cascade analysis with potential flow calculation through a panel method has been used to determine the shock-free inflow condition. The combination between cascade analysis and PSO (particle swarm optimization) algorithm provides an opportunity to develop a diagram of a two-dimensional parameter cascade at various airfoil shapes. Analytical equations have been derived from the diagram that will facilitate the turbomachinery designer in applying the shock-free inflow criterion on their developed cascade. This method has been used to develop the very low head axial hydraulic turbine and provides excellent results of numerical and actual prototype performances.

오목한 반구면의 Jet Impingement/Effusion Hole 주변 유동 특성에 대한 실험과 시뮬레이션의 비교 (Comparison of Experimental and Simulation Results for Flow Characteristics around Jet Impingement/Effusion Hole in Concave Hemispherical Surface)

  • 윤성지;서희림;염은섭
    • 한국가시화정보학회지
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    • 제20권2호
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    • pp.28-37
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    • 2022
  • Flow characteristics of jet impingement over concave hemispherical surface with effusion cooling holes is relatively more complex than that of a flat surface, so the experimental validation for computational fluid dynamics (CFD) results is important. In this study, experimental results were compared with simulation results obtained by assuming different turbulence models. The vortex was observed in the region between the central jets where the recirculation structure appeared. The different patterns of vorticity distributions were observed for each turbulence models due to different interaction of the injected jet flow. Among them, the transition k-kl-ω model predicted similarly not only the jet potential core region with higher velocity, but also the recirculation region between the central jets. From the validation, it may be helpful to accurately predict heat and mass transfer in jet impingement/effusion hole system.

소백산맥에 의한 서풍 파동 발생 (The Generation of Westerly Waves by Sobaek Mountains)

  • 김진욱;윤대옥
    • 한국지구과학회지
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    • 제38권1호
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    • pp.24-34
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    • 2017
  • 등학교에서 사용되는 고급지구과학 교과서에서는 서풍이 대규모 산맥을 넘어갈 때 풍하측에 파동이 발생하는 현상을 개략적인 그림으로 제시하여 간략히 이론적으로만 설명하고 있다. 이 현상은 편서풍 파동 현상으로 산을 넘어가는 공기 기둥의 소용돌이도(잠재와도) 보존 이론으로 설명될 수 있다. 그러나 우리나라와 같이 소규모 산맥이 존재하는 지역에서 관측자료를 바탕으로 중규모 편서풍 파동 현상에 대한 사례 연구는 부재하였다. 또한 서풍에 의한 파동이 형성되는 조건인 산맥의 폭과 길이에 따라 서풍의 풍속, 지속시간을 명확히 규정한 선행연구는 미미하다. 따라서 본 연구에서는 우선적으로 소백산맥을 대상으로 근처의 지표 관측소에서 관측한 지역별 상세관측자료를 이용하여 파동이 실제로 형성되는 지 확인하였다. 또한 소백산맥에 의하여 지표 근처에서 서풍 파동이 생성되기 위한 서풍의 최저속도인 임계 속도를 이론적으로 유도하여, 대략 $0.6m\;s^{-1}$의 값을 구하였다. 더 나아가 기상청 2014년 지역예보모델의 4-차원 자료동화 자료를 추가하여 소백산맥 풍하측 서풍 파동 발생의 연중 빈도와 서풍 파동의 진행 발달과정을 고도별로 분석하였다. 발생한 서풍 파동은 meso-${\beta}$ 또는 -${\gamma}$ 규모였다. 파동의 생성 및 소멸은 풍속 또는 풍향과 밀접한 관계가 있으며, 풍속이 감소함에 따라 산맥에 의한 서풍 파동은 점차 소멸되었다. 서풍이 강할수록 상층에 meso-${\beta}$ 규모의 파장을 갖는 와도 생성 비율이 높았다. 분석 범위를 동아시아 권역으로 넓혔을 때 중국 동북부 옌산 산맥에서도 서풍 파동 현상을 확인할 수 있었다. 본 연구의 결과는 유체지구에 대한 이론과 현상의 이해, 특히 우리나라 산맥에 의해 발생하는 대기의 파동 현상을 실제 관측 자료를 바탕으로 이해를 돕는 교육 자료로 활용될 수 있다.

Global MHD Simulation of a Prolonged Steady Weak Southward Interplanetary Magnetic Field Condition

  • Park, Kyung Sun;Lee, Dae-Young;Kim, Khan-Hyuk
    • Journal of Astronomy and Space Sciences
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    • 제37권2호
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    • pp.77-84
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    • 2020
  • We performed high-resolution three-dimensional global magnetohydrodynamic (MHD) simulations to study the interaction between the Earth's magnetosphere and a prolonged steady southward interplanetary magnetic field (IMF) (Bz = -2nT) and slow solar wind. The simulation results show that dayside magnetic reconnection continuously occurs at the subsolar region where the magnetosheath magnetic field is antiparallel to the geomagnetic field. The plasmoid developed on closed plasma sheet field lines. We found that the vortex was generated at the magnetic equator such as (X, Y) = (7.6, 8.9) RE due to the viscous-like interaction, which was strengthened by dayside reconnection. The magnetic field and plasma properties clearly showed quasiperiodic variations with a period of 8-10 min across the vortex. Additionally, double twin parallel vorticity in the polar region was clearly seen. The peak value of the cross-polar cap potential fluctuated between 17 and 20 kV during the tail reconnection.

Development of a Probability Prediction Model for Tropical Cyclone Genesis in the Northwestern Pacific using the Logistic Regression Method

  • Choi, Ki-Seon;Kang, Ki-Ryong;Kim, Do-Woo;Kim, Tae-Ryong
    • 한국지구과학회지
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    • 제31권5호
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    • pp.454-464
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    • 2010
  • A probability prediction model for tropical cyclone (TC) genesis in the Northwestern Pacific area was developed using the logistic regression method. Total five predictors were used in this model: the lower-level relative vorticity, vertical wind shear, mid-level relative humidity, upper-level equivalent potential temperature, and sea surface temperature (SST). The values for four predictors except for SST were obtained from difference of spatial-averaged value between May and January, and the time average of Ni$\tilde{n}$o-3.4 index from February to April was used to see the SST effect. As a result of prediction for the TC genesis frequency from June to December during 1951 to 2007, the model was capable of predicting that 21 (22) years had higher (lower) frequency than the normal year. The analysis of real data indicated that the number of year with the higher (lower) frequency of TC genesis was 28 (29). The overall predictability was about 75%, and the model reliability was also verified statistically through the cross validation analysis method.

Numerical Experiment on the Sogcho Eddy due to the strong offshore winds in the East Sea

  • Kim Soon Young;Lee Hyong Sun;Lee Jae Chul
    • Fisheries and Aquatic Sciences
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    • 제1권1호
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    • pp.7-18
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    • 1998
  • In order to understand the generation of the Sogcho Eddy due to the strong offshore winds, we first investigated the characteristics of winds at Sogcho, Kangnung and Samchuk, and then carried out a series of numerical experiments using the nonlinear 1 1/2-layer model. The models were forced by wind stress fields, similar in structure to the prevailing winds that a field in the east coast of Korea during the winter season. The winds were composed of the background winds $(-1\;dyne/cm^2)$ for 90 days and the local winds $(-4\;dyne/cm^2)$ for 30 days. The analysis of wind data at three stations (Sogcho, Kangnung, and Samchuk) showed that the wind was stronger in winter than in other seasons and the offshore component was much dominant. According to our numerical solutions, the Sogcho Eddy of about 200 km in diameter was generated due to the strong offshore winds prevailing in the Kangnung - Sogcho regions. The eastward propagation of the Rossby waves reflected at the western boundary resulted in the eastward meandering motion from the eastern side of the eddy.

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태풍 나크리(0208)의 강도변화에 관한 진단적 분석 (A Diagnostic Analysis on the Intensity Change of Typhoon NAKRI(0208))

  • 김백조;김경식;장기호;박종길
    • 한국환경과학회지
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    • 제22권3호
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    • pp.319-329
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    • 2013
  • In this study, the cause of rapid intensity change of typhoon Nakri(0208) in view of point of a trough-typhoon interaction using diagnostic methods was examined based on 6-hourly GDAPS data from 10 to 13 July, 2002. At 0000 UTC 13 July, high PV(Potential Vorticity) region moved southeastward, reaching to the western edge of the Korean peninsula and near typhoon center at surface and there shows an increasing value of EFC(Eddy Momentum Flux Convergence). Also, as the trough and typhoon approach one another at the same time, the vertical shear(850-200 hPa) increases to more than 15 m/s. Thus, it might be concluded that the trough-typhoon interaction made intensified significantly, providing the fact that typhoon Nakri(0208) underwent substantial weakening while moving northward to around Jeju island.

Wiggle Instability of Magnetized Spiral Shocks

  • Kim, Yonghwi;Kim, Woong-Tae
    • 천문학회보
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    • 제39권2호
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    • pp.77.1-77.1
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    • 2014
  • Galactic spiral arms are abundant with interesting gaseous substructures. It has been suggested that arm substructures arise from the wiggle instability (WI) of spiral shocks. While the nature of the WI remained elusive, our recent work without considering magnetic fields shows that the WI is physically originated from the accumulation of potential vorticity (PV) generated by deformed shock fronts. To elucidate the characteristics of the WI in more realistic galactic situations, we extend our previous linear stability analysis of spiral shocks by including magnetic fields. We find that magnetic fields reduce the amount of density compression at shocks, making the shock fronts to move toward the upstream direction. Magnetic tension forces from bent field lines stabilize the WI by prevent the generation of PV. When the spiral-arm forcing is F=5% of the centrifugal force of galaxy rotation, the maximum growth rate of the WI is found to be about 1.0, 0.4, and 0.2 times the orbital angular frequency for the plasma parameter ${\beta}=100$, 10, and 5, respectively. Shocks with ${\beta}=1$ are stable to the WI for F=5%, while becoming still unstable when F=10%.

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