• 상하수도학회지
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• 제23권6호
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• pp.779-788
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• 2009

This study is the result of a field survey of four sewer networks selected from in domestic sanitary sewers. The main purpose of this study is to understand the characteristics of sediment in domestic sanitary sewers and to verify sewer design criteria using minimum Shear Stess for preventing sedimnet. This investigation was carried out at a total of 22 points in the four areas. The characteristics of the sanitary solids that were sampled for suspended solids and bedload matter showed a specific gravity of 1.09, a median particle size of 1.26mm, and 88.9% organic contents. On the other hand, deposited sediment was found at 6 points out of the 22 monitoring points. The analysis results of disposed sediment showed a specific gravity of 2.16, a median particle size of 1.31mm, and 15% organic contents. In flow velocity, the majority of deposited sites have under 0.6m/s. However, one-site which was in large-diameter collector sewers, has recorded over 0.6m/s. The analysis results of tractive force showed that the ability of tractive force has to be $1.5{\sim}2.0N/m^2$ to prevent sediment in domestic Sanitary sewers. In conclusion, to prevent sediment it is necessary to apply a design velocity criteria higher than 0.6m/s in the large diameter collector sewer.

• 지구물리와물리탐사
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• 제15권2호
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• pp.51-56
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• 2012

특정한 지질 구조에 의한 이상을 분리하는 문제, 특히 깊이가 다른 샘들에 의하여 중첩된 이상을 수직적으로 분리하는 문제는 중력과 자력탐사 자료 해석에서 매우 필수적이며 중요한 과정이라 할 수 있다. 측정된 퍼텐셜 자료를 단순하게 광역 효과와 남은 이상의 합으로 가정할 수도 있지만, 수직적으로 여러 층인 구조인 경우로 확장하여 특정한 층에 의한 효과를 분리해 내거나 분리된 이상을 깊이에 관하여 정량적으로 규정할 수 있으면, 이것은 깊이 분리라고 부를 수 있을 것이다. 깊이 분리 필터로서 로그 파워 빛띠 분석을 이용한 진동수 필터를 제안한다. 이것을 수치 모델링과 흥해 일대에서 얻은 실제 중력탐사 자료에 적용하였으며, 2 배 깊이만큼 위로 연속 필터와 비교, 검토해 보았다. 수치 모델링과 실제 중력 자료에 적용한 바에 의하면, 이 논문에서 제안한 깊이 분리 필터는 지구물리적인 의미가 있는 중력 불연속면까지의 중력 효과를 잘 벗겨냄으로써 불연속면의 중력 분포를 추정하여 지질 구조를 해석하는 데에 유용한 도구임을 보여주었다.

• 대한토목학회논문집
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• 제34권2호
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• pp.529-536
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• 2014

점토-시멘트 혼합토의 물리적 특성인 함수비, 비중, 단위중량과 간극비 등은 혼합토의 강도, 압축성, 압밀거동 예측 등에 적용되는 주요한 인자이다. 기존에는 혼합토의 물리적 특성을 복잡한 실내시험 및 시공 후 확인조사를 통해 이루어 졌다. 본 연구는 점토 함수비 90~170%, 시멘트 함유율 5~25%와 재령기간은 3~90일 조건으로 실내시험을 수행하였으며, 양생 후 혼합토 함수비, 비중, 단위중량과 간극비 등에 대한 변화를 분석하였다. 시험결과를 이용하여 원지반 점토 함수비, 시멘트 함유율과 재령기간 등의 역학적 관계를 바탕으로 혼합토의 함수비, 비중과 단위중량에 관한 물성 예측식을 제안하였다. 혼합토의 물성 예측식을 지반공학 분야에서 일반적으로 사용하는 간극비 산출식에 대입하여 혼합토의 간극비 예측식을 도출하였으며, 방콕 점토를 대상으로 간극비에 대한 실험결과와 본 연구에서 제안한 예측식을 검증하였다.

• 대한기계학회논문집B
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• 제29권9호
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• pp.997-1005
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• 2005

The extinction characteristics of low strain rate normal gravity (1-g) nonpremixed methane-air flames were studied numerically and experimentally. A time-dependent axisymmetric two-dimensional (2D) model considering buoyancy effects and radiative heat transfer was developed to capture the structure and extinction limits of 1-g flames. One-dimensional (1D) computations were also conducted to provide information on 0-g flames. A 3-step global reaction mechanism was used in both the 1D and 2D computations to predict the measured extinction limit and flame temperature. A specific maximum heat release rate was introduced to quantify the local flame strength and to elucidate the extinction mechanism. Overall fractional contribution by each term in the energy equation to the heat release was evaluated to investigate the multi-dimensional structure and radiative extinction of 1-g flames. Images of flames were taken for comparison with the model calculation undergoing extinction. The two-dimensional numerical model was validated by comparing flame temperature profiles and extinction limits with experiments and ID computation results. The 2D computations yielded insight into the extinction mode and flame structure of 1-g flames. Two combustion regimes depending on the extinction mode were identified. Lateral heat loss effects and multi-dimensional flame structure were also found. At low strain rates of 1-g flame ('Regime A'), the flame is extinguished from the weak outer flame edge, which is attributed to multi-dimensional flame structure and flow field. At high strain rates, ('Regime B'), the flame extinction initiates near the flame centerline due to an increased diluent concentration in reaction zone, which is the same as the extinction mode of 1D flame. These two extinction modes could be clearly explained with the specific maximum heat release rate.

• Earthquakes and Structures
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• 제18권2호
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• pp.201-213
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• 2020

Seismic damages that occurred by the effects of epicenter distance of the earthquake are one of the most important problems for the earthquake engineering. In this study, it is aimed to examine the nonlinear seismic behaviors of concrete gravity (CG) dams considering various epicenter distances. For this purpose, Boyabat CG dam that is one of the biggest concrete gravity dams in Turkey is selected as a numerical application. FLAC3D software based on finite difference method is used for modelling and analyzing of the dam. Drucker-Prager nonlinear material model is used for the concrete body and Mohr-Coulomb nonlinear material model is taken into account for the foundation. Special interface elements are used between dam body and foundation to represent interaction condition. Free-field and quiet non-reflecting boundary conditions are utilized for the main surfaces of 3D model. Total 5 various epicenter distances of 1989 Loma Prieta earthquake are considered in 3D earthquake analyses and these distances are 5 km, 11 km, 24 km, 85 km and 93 km, respectively. According to 3D seismic results, x-y-z displacements, principal stresses and shear strain failures of the dam are evaluated in detail. It is clearly seen from this study that the nonlinear seismic behaviors of the CG dams change depending to epicenter distance of the earthquake. Thus, it is clearly recommended in this study that when a CG dam is modelled or analyzed, distance of the earthquake fault to the dam should be strongly examined in detail. Otherwise, earthquake damages can be occurred in the concrete dam body by the effects of seismic loads.

• 한국지구물리탐사학회:학술대회논문집
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• 한국지구물리탐사학회 2003년도 Proceedings of the international symposium on the fusion technology
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• pp.142-149
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• 2003

Blind hydraulic backfilling is a commonly used technique for subsidence control of the strata over unapproachable waterlogged underground excavations. In this investigation model studies on all the three variants of this technique, namely, hydro-pneumatic or air-assisted gravity backfilling, pumped-slurry backfilling and simple gravity backfilling, have been carried out in fully transparent models of the underground excavations. On examination of the filling process, it was revealed that in all the three cases, the basic process of filling occurs by sand transport along one or more meandering channels. The relative influence of sand, water and air flow rates on the area of filling from a single inlet point and the hydraulic pressure loss per unit length were studied in details. In hydro-pneumatic backfilling process, the air bubbles while moving upward through the meandering channels provide an additional buoyant force over and above the available hydraulic head. In this way the area of filling from a single borehole may be quite large even at small flow rates of water. During actual field implementation the injected air, if not released completely from the rise side holes, may cause troubles by way of creating potholes on the surface. The pumped-slurry technique has shown its capability of filling a relatively larger area at faster rate, especially when high-volume, low-pressure method was selected. But simple gravity filling was also found to be equally effective method as slurry pumping, especially when flow rates were high. In the second and third method discussed above, examination of variations of injection pressure was also done and its relation with physical phenomenon was also attempted. Some empirical relationships were also developed using multivariate regression with a view to help the practicing engineers.

• 한국지반공학회지:지반
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• 제13권4호
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• pp.135-148
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• 1997

옹벽에 작용하는 토압을 구하기 위하여 Coulomb이론이 실무에 대부분 사용되고 있지만, 전수평토압의 작용위치를 구할 수 없으므로 토압분포를 삼각형 분포라고 가정하고 있다. 그러나, 수 많은 실내 및 현장실험을 통하여 토압분포가 그렇지 않다는 것으로 규명되었다. 이러한 문제를 극복하기 위한 이론적인 접근이 Handy(1985), Kingsley(1989), Kellogg(1993), 정성교(1993, 1996a) 등에 의하여 비 점성토로 뒤채움된 옹벽에 대하여 수행되었다. 점성토로 뒤채움된 옹벽에 대한 기존의 이론적 접근은 단지 Rankine또는 Coulomb 이론에 근거하여 주로 수행되었지만, 그 이론들은 제각기 다른 결과를 보여주었다. 여기서는 점성토로 뒤채움된 중력식옹벽에 작용하는 수평토압을 위한 이론적 접근이 비배수 조건하에서 수행되었다. 이 접근은 Coulomb의 가정에 바탕을 두고 아칭개념을도입하였으며, 인장균열을 무시한 경우와 고려한 경우에 대하여 각각 이론식이 유도되었다. 그리고, 몇가지 조건에 대한 비교결과에서 인장균열을 고려한 토압이론식의 적용이 합리적일 것으로 사료되었다.

• 천문학회지
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• 제24권2호
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• pp.129-149
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• 1991

An attempt has been made to examine the characteristics of acoustic and MHD waves generated in stellar convection zones($4000\;K\;{\leq}\;T_{eff}\;{\leq}\;7000\;K$, $3\;{\leq}\;\log\;g\;{\leq}\;4.5$). With the use of wave generation theories formulated for acoustic waves by Stein (1967), for MHD body waves by Musielak and Rosner (1987, 1988) and for MHD tube waves by Musielak et al.(l989a, 1989b), the energy fluxes are calculated and their dependence on effective temperature, surface gravity and megnetic field strength are analyzed by optimization techniques. In computing magneto-convection models, the effect of magnetic fields on the efficiency of convection has been taking into account by extrapolating it from Yun's sunspot models(1968; 1970). Our study shows that acoustic wave fluxes are dominant in F and G stars, while the MHD waves dominant in K and M stars, and that the MHD wave fluxes vary as $T_{eff}^4{\sim}T_{eff}^7$ in contrast to the acoustic fluxes, as $T_{eff}^{10}$. The gravity dependence, on the other hand, is found to be relatively weak; the acoustic wave fluxes ${\varpropto}\;g^{-0.5}$, the longitudinal tube wave fluxes ${\varpropto}\;g^{0.3}$ and the transverse tube wave fluxes ${\varpropto}\;g^{0.3}$. In the case of the MHD body waves their gravity dependence is found to be nearly negligible. Finally we assesed the computed energy fluxes by comparing them with the observed fluxes $F_{ob}$ of CIV(${\lambda}1549$) lines and soft X-rays for selected main sequence stars. When we scaled the corrected wave fluxes down to $F_{ob}$, it is found that these slopes are almost in line with each other.

• Earthquakes and Structures
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• 제25권2호
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• pp.125-134
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• 2023

In the present work, a new global damage index is proposed for the seismic performance and failure analysis of concrete gravity dams. Unlike the existing indices of concrete structures, this index doesn't need scaling with an ultimate or an upper value. For this purpose, the Beni-Haroun dam in north-eastern Algeria, is considered as a case study, for which an average seismic capacity curve is first evaluated by performing several incremental dynamic analyses. The seismic performance point of the dam is then determined using the N2 method, considering multiple modes and taking into account the stiffness degradation. The seismic demand is obtained from the design spectrum of the Algerian seismic regulations. A series of recorded and artificial accelerograms are used as dynamic loads to evaluate the nonlinear responses of the dam. The nonlinear behaviour of the concrete mass is modelled by using continuum damage mechanics, where material damage is represented by a scalar field damage variable. This modelling, which is suitable for cyclic loading, uses only a single damage parameter to describe the stiffness degradation of the concrete. The hydrodynamic and the sediment pressures are included in the analyses. The obtained results show that the proposed damage index faithfully describes the successive brittle failures of the dam which increase with increasing applied ground accelerations. It is found that minor damage can occur for ground accelerations less than 0.3 g, and complete failure can be caused by accelerations greater than 0.45 g.

• Journal of Astronomy and Space Sciences
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• 제8권1호
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• pp.85-98
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• 1991

지구의 남극과 북극 주위를 저고도로 돌고 있는 소형 과학위성의 자세 조정을 위해 지구자기장을 이용하였다. 이것을 위해 소형 과학위성의 Telemetry 자료를 분석하였다. 위성에 장치된 3축 magnetometer에서 자기장 성분의 크기와 변동량을 측정하여 위성의 회전상태를 알아내는 방법이 제시되었다. 위성이 회전축에 대하여 대칭형인 경우 특정한 위치에서의 자세판단이 가능하다. 현재 자세와 원하는 자세를 비교했을 때 나타나는 차이를 각 축에 대한 회전속도의 조절로 제거할 수 있는 방법을 연구하였다. 여기에서는 자세 측정으로부터 얻은 자료를 가지고 magnetorquer에 공급되어야 할 전류의 크기(혹은 유지시간)를 계산하는 기본 알고리즘을 연구하였고 직접 프로그램으로 작성해서 수행시켜 보았다. 이러한 자세제어 방법은 위성이 초기 tumbling 운동을 할 때와 Gravity gradient boom에 의한 수동제어가 이루어진 후에 적용할 수 있다.