• 제목/요약/키워드: Continuum Mechanism

검색결과 47건 처리시간 0.025초

Strut-and-tie model of deep beams with web openings - An optimization approach

  • Guan, Hong
    • Structural Engineering and Mechanics
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    • 제19권4호
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    • pp.361-379
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    • 2005
  • Reinforced concrete deep beams have useful applications in tall buildings and foundations. Over the past two decades, numerous design models for deep beams were suggested. However even the latest design manuals still offer little insight into the design of deep beams in particular when complexities exist in the beams like web openings. A method commonly suggested for the design of deep beams with openings is the strut-and-tie model which is primarily used to represent the actual load transfer mechanism in a structural concrete member under ultimate load. In the present study, the development of the strut-and-tie model is transformed to the topology optimization problem of continuum structures. During the optimization process, both the stress and displacement constraints are satisfied and the performance of progressive topologies is evaluated. The influences on the strut-and-tie model in relation to different size, location and number of openings, as well as different loading and support conditions in deep beams are examined in some detail. In all, eleven deep beams with web openings are optimized and compared in nine groups. The optimal strut-and-tie models achieved are also compared with published experimental crack patterns. Numerical results have shown to confirm the experimental observations and to efficiently represent the load transfer mechanism in concrete deep beams with openings under ultimate load.

시이펏 은하 NGC 5728의 OASIS 분광 영상 (OASIS Spectral Images of the Seyfert galaxy NGC 5728)

  • 형식;송동훈;;이우백
    • 한국지구과학회지
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    • 제27권5호
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    • pp.569-578
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    • 2006
  • CFHT 천문대 3.6 m 망원경에 부착된 OASIS 분광기를 사용하여 얻은 자료로부터 continuum, $H{\alpha},\;H{\beta}$, [O III], [N II] 등의 영상을 만들어 활동 은하핵 NGC 5728의 물리적 특성을 분석하였다. NGC 5728의 중심부에 NLR 영역으로 판단되는 약 $15"{\times}12"$ 범위 영역에 3개의 밝은 부분(NW knot, SE knot, nucleus)이 존재하고 있고, 이는 핵(nucleus)을 중심으로 북서방향이나 서쪽으로 물질의 흐름이 일어나고 있음을 암시한다. 우리는 직경 10"인 ring과 이의중심에 있는 NW knot의 구조가 은하중심과 일치하지 않음을 발견하였다. 우리는 이러한 구조의 생성 원인에 대해 알아보기 위하여 핵과 knot의 운동학적 특성을 비교하여 보았고, 방출선 영상에서 보이는 차이점을 비교함으로써 활동 은하 중심부의 구조를 살펴보았다.

주기편측간질모양방전은 발작현상이 아니라 단지 급성 뇌손상을 반영하는 것이다 (Periodic Lateralized Epileptiform Discharges Are Not Ictal Phenomenon, and Just Reflect an Acute Brain Damage)

  • 이상암
    • Annals of Clinical Neurophysiology
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    • 제13권1호
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    • pp.26-30
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    • 2011
  • Although the pathophysiologic mechanism is unknown, there has been long-running debate on whether periodic discharges such as periodic lateralized epileptiform discharges (PLEDs) and generalized periodic epileptiform discharges are an ictal or interictal EEG pattern. The goal of this review is to give evidence that such periodic discharges on EEG are not ictal phenomenon and just represent underlying acute brain damage. This review includes coma with epileptiform EEG pattern and its prognostic and therapeutic implications. Based on previous reports, rather than taking the view PLEDs represent either an underlying ictal process or an electrographic correlate of neuronal injury, it would be more reasonable that PLEDs are considered as a dynamic pathophysiological state in which unstable neurobiological processes create an ictal-interictal continuum.

CLUSTER MERGERS AND NON-THERMAL PHENOMENA: A STATISTICAL MAGNETO-TURBULENT MODEL

  • CASSANO R.;BRUNETTI G.
    • 천문학회지
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    • 제37권5호
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    • pp.583-587
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    • 2004
  • With the aim to investigate the statistical properties and the connection between thermal and non-thermal properties of the ICM in galaxy clusters, we have developed a statistical magneto-turbulent model which describes, at the same time, the evolution of the thermal and non-thermal emission from galaxy clusters. In particular, starting from the cosmological evolution of clusters, we follow cluster. mergers, calculate the spectrum of the magnetosonic waves generated in the ICM during these mergers, the evolution of relativistic electrons and the resulting synchrotron and Inverse Compton spectra. We show that the broad band (radio and hard x-ray) non-thermal spectral properties of galaxy clusters can be well accounted for by our model for viable values of the parameters (here we adopt a EdS cosmology).

PARTICLE ACCELERATION AND NON-THERMAL EMISSION FROM GALAXY CLUSTERS

  • BRUNETTI GIANFRANCO
    • 천문학회지
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    • 제37권5호
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    • pp.493-500
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    • 2004
  • The existence and extent of non-thermal phenomena in galaxy clusters is now well established. A key question in our understanding of these phenomena is the origin of the relativistic electrons which may be constrained by the modelling of the fine radio properties of radio halos and of their statistics. In this paper we argue that present data favour a scenario in which the emitting electrons in the intracluster medium (ICM) are reaccelerated in situ on their way out. An overview of turbulent-particle acceleration models is given focussing on recent time-dependent calculations which include a full coupling between particles and MHD waves.

"Dust, Ice, and Gas In Time" (DIGIT) Herschel observations of GSS30-IRS1

  • Je, Hyerin;Lee, Jeong-Eun
    • 천문학회보
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    • 제38권2호
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    • pp.66.2-66.2
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    • 2013
  • As part of the DIGIT key program, we observed GSS30-IRS1, a Class I object located in Ophiuchus (d=125 pc), with Herschel-PACS. More than 70 lines were detected in 50-200 micron band including CO, OH, H2O, and [OI]. All lines, except for [OI], were detected only at the central spaxel of $9.4^{{\prime}{\prime}}{\times}9.4^{{\prime}{\prime}}$ while the [OI] emission is extended along the NE-SW direction. One interesting feature in GSS30-IRS1 is that the continuum is extended beyond PSF, unlike line emission. It suggests that the external heating is important in GSS30-IRS1. For detail analysis of line fluxes, we apply the non-LTE LVG model, RADEX as well as simple rotational diagrams. We also use the Monte Carlo radiative transfer package, RADMC-3D to understand the heating mechanism of dust grains around GSS30-IRS1. We will discuss about heating and cooling processes associated with GSS30-IRS1.

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단섬유 금속복합재료의 응력-변형률 히스테리시스 거동 해석 (Analysis of Stress-Strain Hysteresis Behavior in Metal Composites)

  • 김홍건
    • 한국공작기계학회:학술대회논문집
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    • 한국공작기계학회 1997년도 추계학술대회 논문집
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    • pp.132-139
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    • 1997
  • The strengthening mechanism of short fiber or whisker reinforced metal matrix composites has been studied by a continuum mechanics treatment utilizing finite element analysis (FEM). To assess the tensile and compressive constitutive responses, a constraint-unconstraint comparative study based on stree-strain hysteresis loop has been performed. For analysis procedures, the aligned axisymmetric single fiber model and the stress grouping technique have been implemented to evaluate the domain-based field quantities. Results indicated that the development of significant triaxial stresses within the matrix both for the tensile and compressive loading, due to the constraint imposed by reinforcements, provides and important contribution to strengthening. It was also found that fiber stresses are not only sensitive to the fiber/fiber interaction effects but also substantially contribute to the composite strengthening both for the tensile and compressive loading.

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Configuration sensitivity analysis of mechanical dynamics

  • Bae, Daesung
    • 한국공작기계학회논문집
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    • 제10권1호
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    • pp.112-119
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    • 2001
  • Design sensitivity is an important is an important device in improving a mechanical system design. A continuum design consists of the shape and orientation design. This research develops the shape and orientation design sensitivity method. The configura-tion design variables of multibody systems define the shape and orientation changes. The equations of motion are directly differentiated to obtain the governing equations for the design sensitivity. The governing equation of the design sensitivity is formulated as an over determined differential algebraic equation and treated as ordinary differential equations on mani-folds. The material derivative of a domain functional is performed to obtain the sensitivity due to shape and orientation changes. The configuration design sensitivities of a fly-ball governor system and a spatial four bar mechanism are obtained using the proposed method and are validated against those obtained from the finite difference method.

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취성재의 결함을 고려한 파괴기준에 대한 연구 (Failure Criterion Including Brittle Damage)

  • 여은구;이용신
    • 대한기계학회:학술대회논문집
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    • 대한기계학회 2001년도 춘계학술대회논문집A
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    • pp.507-510
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    • 2001
  • Brittle failure mechanism has been well known as growth of initial micro-damage, that causes macro crack and failure in the end. Several precise criteria are suggested recently, based on experiments values in a whole load range. Among them, Mohr-Coulomb's criterion is used widely these days, but it has a big error compared with the real failure behavior since it does not show reciprocal actions of stresses. In this study, a new brittle failure criterion is proposed, which includes the effects of brittle damage evolution by taking a brittle damage parameter specifically. Comparisons between the proposed model and the previous ones are also given.

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흐름효과를 고려한 액정의 시뮬레이션 (Simulation of Liquid Crystals Considering Flow Effect)

  • 김훈;박우상
    • 한국전기전자재료학회논문지
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    • 제19권3호
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    • pp.260-266
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    • 2006
  • In this paper, We coupled fluid balance and director balance equation from Ericksen-Leslie's continuum theory and observed the motion of Liquid Crystal molecular. We simulated flow velocity and director distribution in which flow effect is considered in switching on and switching off state. We interpreted the dynamic response characteristic caused by the flow. As the result of the simulation, We could see the flow effect. In the case of Twisted Nematic(TN) cell, this flow caused abnormal twist temporarily in switching off state. We could prove that this abnormal twist is a direct cause of optical bounce phenomenon known well until now with the result of simulation. In addition, We analyzed the mechanism of the fast response due to flow in the case of Optically Compensated Bend(OCB) cell.