• 제목/요약/키워드: Continuum distribution

검색결과 158건 처리시간 0.034초

Development and Application of Two-Dimensional Hydrogen Mixing Model in Containment Subcompartment Under Severe Accidents

  • Lee, Byung-Chul;Cho, Jae-Seon;Park, Goon-Cherl;Chung, Chang-Hyun
    • Nuclear Engineering and Technology
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    • 제29권2호
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    • pp.110-126
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    • 1997
  • A two-dimensional continuum model for the hydrogen mining phenomena in the containment subcompartment under severe accident conditions has been developed to predict the spatial distribution of the hydrogen concentration. The model can predict the distribution of time-dependent hydrogen concentration for HEDL experiments well. For the simulation of these experiments, the hydrogen is mixed uniform within the test compartment. To predict the extent of non-uniform distribution, the dominant factors such as the geometrical shape of obstacle and velocity of source injection in mixing phenomena are investigated. If the obstacle disturbing the flow of gas mixture exists in the compartment, the uniform distribution of hydrogen might be not guaranteed. The convective circulation of gas flow is separately formed up and down of the obstacle position, which makes a difference of hydrogen concentration between the upper and lower region of the compartment. The recirculation flow must have a considerable mass flow rate relative to velocity of the source injection to sustain the well-mixed conditions of hydrogen. Finally, in order to account for non-uniform distribution of the hydrogen due to the geometrical configuration the maximum-to-average ratio is functionalized.

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THE DISTRIBUTION MODELS OF THERMAL AND NON-THERMAL RADIO CONTINUUM EMISSION IN THE GALACTIC DISK

  • SANGUANSAK N.;OSBORNE J. L.
    • 천문학회지
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    • 제29권spc1호
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    • pp.169-170
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    • 1996
  • In the past, it. was very difficult to distinguish thermal and non-thermal emission. Broadbent et a1. (1989) has developed a new technique with the help of the IRAS 60 micron emission. The distribution of non-thermal or synchrotron emission in the Galactic disk has been modeled from the 408 MHz all sky survey of Haslam et a1. (1982) after removal of the thermal component.. At. 408 MHz, t.here is very little absorption in the interstellar medium and the distribution along the line-of-sight. is inferred mainly from its presumed relationship to other tracers of spiral structure via a. number of fitted parameters. But. at lower frequencies, free-free absorption becomes important and can give some direct. information on the line of sight. distribution. We have modeled the thermal electron density according to the spiral arm models and the distribution of ionized hydrogen in the Galactic plane by Lockman (1976) and Cersosimo et. al. (1989) and have made predictions to compare with the surveys of Dwarakanath et al. (1990) at. 34.5 MHz and .Jones and Finlay (1974) at 29.9 MHz. The result confirms that the absorption model of the synchrotron emissivity in the Galactic plane is broadly corrected and illustrates the potential of the absorption technique.

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내부튜브가 있는 골조 튜브 구조물의 전단응력에 대한 수치해석 (Numerical Analysis of Shear Stresses in Framed Tube Structures with Internal Tube(s))

  • 이강건;이리형
    • 한국전산구조공학회논문집
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    • 제15권3호
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    • pp.511-521
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    • 2002
  • 내부튜브를 가진 튜브 구조물의 보에 있는 전단응력을 평가하기 위하여 수치적인 해석기법이 제안되었다 이 기법은 휨과 전단변형을 고려한 튜브 보 개념 위에서 각각의 튜브를 연속 보로서 모델링 한다. 전단응력에 대한 수치해석은 패널에 작용하는 응력에 대한 탄성이론과 수학적인 유도를 기초로 하고 있다. 내부와 외부 튜브에 있는 변형곡선에 대한 표현식을 가정함으로써, 그 튜브에 있는 전단응력은 작용하중과 단면 2차 모멘트 그리고 구조물의 기하학적인 표현으로 구성된 선형 함수로서 표현된다 전단지체와 축 응력을 다룬 이전의 연구가 튜브내에 존재하는 전단응력을 수치적으로 해석하기 위하여 보완 발전되었다. 제안된 방법의 정확성과 유용성이 3개의 튜브 구조물의 해석을 통하여 증명 되었다

연속체 절리모델을 이용한 불연속성암반 내 지하공동의 변형거동에 관한 수치해석 (Numerical Analysis of Deformation Behaviour of Underground Opening in a Discontinuous Rock Mass Using a Continuum Joint Model)

  • 강상수;이종길;백환조
    • 지질공학
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    • 제15권3호
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    • pp.257-268
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    • 2005
  • 일반적으로 현지 암반은 강도의 변화가 심 한 다양한 불연속면들을 포함하여 불균질하고 불연속성 을 나타낸다. 절리, 단층, 균열, 층리와 같은 불연속면들은 암반의 강도와 변형특성을 좌우하는 중요한 요인이다. 결과적으로, 지하공동의 안정성은 무결암의 역학적 특성뿐만 아니 라, 공동의 기하학적 형상과 관련하여 불연속면들의 공간적 분포와 역학적 특성에 크게 영 향을 받는다. 따라서 지하심부의 응력 조건에서의 공동설계를 위해서는 불연속 암반의 거동에 대한 정확한 이해가 필수적이다. 암반역 학 분야의 발전에 의하여 등방성 암반에서 의지 하공동 설계를 위한 기준이 제시되고 있으나, 불연속성 암반의 변형 거동은 불명확성 이 여전히 존재한다. 본 연구에서는 연속체절 리모델을 적용하여 불연속성 암반내의 지하공동 주변의 소성영역의 크기, 응력분포 및 변형거동에 대하여 매개변수의 변화에 따른 영향을 고찰하였다. Mohr-Coulomb 파괴 이론에 의한 탄소성 유한차분법을 적용하였으며, 비조합 유동법칙과 완전소성 물질거 동을 가정하였다.

THE DISTRIBUTION OF DUST INSIDE THE ORION NEBULA

  • Shin, Jun-Ho;Hong, Seung-Soo
    • 천문학회지
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    • 제20권1호
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    • pp.1-26
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    • 1987
  • By inverting the brightness integral for the dust-scattered continuum, we have determined how the dust grains are distributed inside the Orion nebula. The scattering characteristics of the Orion dust at a given wavelength is kept constant within the nebula, and the geometry of the nebula is assumed to have a hemispherical shape. The resulting radial distance dependence of the distribution of dust number density, $N_d(r)$, shows that the dust grains are depleted at the central region of the Orion nebula and concentrated in the region $5'{\sim}6'$ away from the Trapezium stars. The scattering characteristics of the Orion dust are of moderately forward throwing nature, and the Orion dust has low values of albedo.

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POLARIZATION OF FIR EMISSION FROM T TAURI DISKS

  • Cho, Jung-Yeon;Lazarian, A.
    • 천문학회지
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    • 제40권4호
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    • pp.113-118
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    • 2007
  • Recently far infra-red (FIR) polarization of the $850{\mu}m$ continuum emission from T Tauri disks has been detected. The observed degree of polarization is around 3 %. Since thermal emission from dust grains dominates the spectral energy distribution at the FIR regime, dust grains might be the cause of the polarization. We explore alignment of dust grains by radiative torque in T Tauri disks and provide predictions for polarized emission for disks viewed at different wavelengths and viewing angles. In the presence of magnetic field, these aligned grains produce polarized emission in infrared wavelengths. When we take a Mathis-Rumpl-Nordsieck-type distribution with maximum grain size of $500-1000{\mu}m$, the degree of polarization is around 2-3 % level at wavelengths larger than ${\sim}100{\mu}m$. Our study indicates that multifrequency infrared polarimetric studies of protostellar disks can provide good insights into the details of their magnetic structure.

암석절리와 균열망내에서의 채널흐름에 관한 이론적 수치해석적 연구 (A Theoretical and Numerical Study on Channel Flow in Rock Joints and Fracture Networks)

  • 송명규;주광수
    • 터널과지하공간
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    • 제4권1호
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    • pp.1-16
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    • 1994
  • The study on the flow characteristics and analysis of groundwater in discontinuous rock mass is very important, since the water inflow into the underground opening during excavation induces serious stability and environmental problems. To investigate the flow through single rock joint, the effect of various aperture distribution on the groundwater flow has been analyzed. Observed through the analysis is the "channel flow", the phenomenon that the flow is dominant along the path of large aperture for given joint. The equivalent hydraulic conductivity is estimated and verified through the application of the joint network analysis for 100 joint maps generated statistically. Both the analytic aproach based on isotropic continuum premise and the joint network analysis are tested and compared analyzing the gorundwater inflow for underground openings of different sizes and varying joint density. The joint network analysis is considered better to reflect the geometric properties of joint distribution in analyzing the groundwater flow.ater flow.

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최적조건법에 의한 위상 최적화 연구 (Topology Optimization using an Optimality Criteria Method)

  • 김병수;서명원
    • 한국자동차공학회논문집
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    • 제7권8호
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    • pp.224-232
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    • 1999
  • Topology optimization has evolved into a very efficient concept design tool and has been incorporated into design engineering processes in many industrial sectors. In recent years, topology optimization has become the focus of structural design community and has been researched and applied widely both in academia and industry. There are mainly tow approaches for topology optimization of continuum structures ; homogenization and density methods. The homogenization method is to compute is to compute an optimal distribution of microstructures in a given design domain. The sizes of the micro-calvities are treated as design variables for the topology optimization problem. the density method is to compute an optimal distribution of an isotropic material, where the material densities are treated as design variables. In this paper, the density method is used to formulate the topology optimization problem. This optimization problem is solved by using an optimality criteria method. Several example problems are solved to show the usefulness of the present approach.

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춘성지구 북한강유역의 지하수위에 따른 식물군락의 운적적 변화 (The Distribution of Plant Communities on Water Table along the Bukhan Riverside in Chun-seong)

  • 이성규
    • Journal of Plant Biology
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    • 제16권3_4호
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    • pp.1-6
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    • 1973
  • The distribution of plant communities along the Bukhan Riverside in Chun-seong was studied by means of the methods fo Curtis and Pattern. The communities were arranged in a single-dimensioned ordination on the basis of the importance values of the persistent species. Leading dominant species, form the 'low' level to the 'high' levels of the ordination gradient, were Phalaris arundinacea, Salix gilgiana, Artemisia feddei, Zoysia japonica, Pennisetum japonicum, and Arundinella hirta. These species from a continuum from the river to the dry grassland depending upon available soil-moisture. Standing crops in terms of dry weight and the nitrogen content of the above-ground parts of these species showed a good relationship with gradients of available soil-moisture.

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Recent Development of Analytical Solutions to Brownian Aerosol Coagulation in Different Particle Size Regimes

  • Park, Seong-Hun;Kim, Hyun-Tae;Lee, Kyoo-Won
    • Journal of Korean Society for Atmospheric Environment
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    • 제15권E호
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    • pp.65-71
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    • 1999
  • The log-normal size distribution theories developed recently for aerosol coagulation are reviewed. The analytical solutiosn to Brownian coagulation developed recently for various particle size regimes are reviewed. In order to describe the evolution of the size distribution of a coagulating aerosol over the entire size range, the analytical solutions developed individually for the free-molecule regime, the transition regime, the nearcontinuum regime, and the continuum regime have been combined. The work described here represents the first analytical solution to the aerosol coagulation problem covering the entire particle size range.

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