• 터널과지하공간
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• 제10권1호
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• pp.33-44
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• 2000

이 연구에서는 지하공동의 점진적인 붕락이 지표침하에 미치는 영향을 조사하기 위하여, 주문진산 표준사를 이용하여 모형지반을 구성하였으며, 공동의 심도를 달리하는 6가지 모델에 대하여 실내 모형실험을실시하였다. 여기서 공동의 심도와 붕락구간의 크기에 따른 침하발생양상을 조사하였다. 또한 NCB 방법, 지수함수를 이용한 윤곽함수법 영향함수법 등의 침하예측방법을 이용하여 모형실험으로부터 측정된 수직 및 수평변위를 해석하였으며, 모래지반에 적합한 침하예측방법을 제안하였다.

• 한국안전학회지
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• 제22권3호
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• pp.74-80
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• 2007

In this study, a documentary survey, face mapping, and stability analysis were performed on the collapsed colluvial soil slope. The purpose of this paper is to identify the cause of slope failure and determine slope stability for similar areas. Boring samples were extracted from the slump and laboratory tests were performed to find out the cause of slope failure. In addition, the limit equilibrium method was used in order to determine the stability of the slope. As a result of this investigation and the analysis of data, the type of collapse and cause of slope failure have been shown to have a strong correlation with the natural geographical and geological features which make up the collapse profile of the study area. These results will help to develop guidelines for formulating countermeasure methods.

• 천문학회지
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• 제29권spc1호
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• pp.139-140
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• 1996

• 천문학회보
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• 제41권2호
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• pp.54.3-55
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• 2016

We model the spectral energy distribution (SED) of the Class 0 protostar L1527 IRS using a dust continuum radiative transfer code RADMC-3D to study the initial condition of gravitational collapse. To constrain the envelope structure, we use the data obtained by Herschel /PACS, which covers the far-infrared regime ($55-190{\mu}m$) where the SED of L1527 IRS peaks. According to our modeling, a more flattened density profile fits the far-infrared SED of L1527 IRS better than the density profile of a rotating and infalling envelope. Thus, we employ the density structure of a Bonnor-Ebert sphere, which consists of the inner flat-topped and the outer power-law regions and is often used for describing the density structure of the youngest sources in the low mass star formation process. A Bonnor-Ebert sphere fits very well the observed SED at ${\lambda}$ > $10{\mu}m$, suggesting that L1527 IRS might collapse from an unstable Bonnor-Ebert sphere rather than a singular isothermal sphere.

• 대한화학회지
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• 제28권3호
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• pp.185-193
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• 1984

송아지 胸線 DNA의 nucleotide 당 spermine 0.016 분자의 비율로 結合되는 spermine 濃度에서 그 DNA와 ethidium과의 結合에 對한 Hill 係數는 1.7인 反面에 spermine이 存在하지 않는 條件에서는 그 Hill 係數가 0.38이었다. Spermine에 依한 DNA의 viscometric titration data, 260nm에서의 anomalous absorbance-temperature profile 및 粘性度-溫度 樣相과 더불어 이 data를 基礎로 하여 spermine 結合에 依하여 誘發되는 conformational transition의 allosteric propagation이 DNA의 凝縮된 構造로의 單分子的 collapse에 관여됨을 豫測할 수 있다.

• Journal of Astronomy and Space Sciences
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• 제4권1호
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• pp.1-10
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• 1987

Results of N-body simulation of dissipationless cold collapse of spherical gravitating system are presented. We compared the results with properties of elliptical. The system gradually evolved to triaxial system. The projected density profile is in good agreement with the de Vaucouleur's r¼ law and the velocity dispersion profile is consistent with observations. In addition to triaxial instability, it seems that there is another instability.

• Geomechanics and Engineering
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• 제16권6호
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• pp.569-575
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• 2018

The stability of shallow cavities with an arbitrary profile is a difficult issue in geotechnical engineering. This paper investigates this problem on the basis of the upper bound theorem of limit analysis and the Hoek-Brown failure criterion. The influence of pore pressure is taken into consideration by regarding it as an external force acting on rock skeleton. An objective function is constructed by equating the internal energy dissipation to the external force work. Then the Lagrange variation approach is used to solve this function. The validity of the proposed method is demonstrated by comparing the analytical solutions with the published research. The relations between shallow and deep cavity are revealed as well. The detaching curve of cavity roof with elliptical profile is obtained. In order to facilitate the application of engineering practice, the numerical results are tabulated, which play an important role in tunnel design and stability analysis of roof. The influential factors on potential collapse are taken into consideration. From the results, the impact of various factors on the extent of detaching is seen intuitively.

• 구강회복응용과학지
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• 제31권3호
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• pp.262-272
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• 2015

구치부 교합지지 상실과 비정상적 악간 관계는 교합 부조화로 이어지며 다양한 병적 징후를 동반한다. 저작, 심미 및 발음 기능을 회복하기 위해 교합고경과 교합평면 재설정에 따른 완전구강회복이 필요하게 된다. 본 증례는 75세의 여성으로 교합지지 상실과 불균일한 교합평면 및 II 급 부정교합을 가지고 있었다. 안모를 관찰하고 악간관계를 평가한 결과 상하악의 최대교두간접촉위가 상실되면서 수직교합고경이 감소된 것으로 진단되었다. 상악 국소의치와 하악 고정성보철물로 상실된 교합수직고경을 회복하고 조화로운 교합평면을 형성하였다. 수직고경 거상량은 7.5 mm로 하였고, 임시보철물을 이용하여 8 주간 경과 관찰 후 최종 보철물을 제작하였으며 저작효율과 심미성은 개선되었다.

• 대한치과교정학회지
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• 제49권1호
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• pp.59-69
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• 2019

In this report, we describe a case involving a 34-year-old woman who showed good treatment outcomes with long-term stability after multidisciplinary treatment for unilateral cleft lip and palate (CLP), maxillary hypoplasia, severe maxillary arch constriction, severe occlusal collapse, and gingival recession. A comprehensive treatment approach was developed with maximum consideration of strong scar constriction and gingival recession; it included minimum maxillary arch expansion, maxillary advancement by distraction osteogenesis using an internal distraction device, and mandibular setback using sagittal split ramus osteotomy. Her post-treatment records demonstrated a balanced facial profile and occlusion with improved facial symmetry. The patient's profile was dramatically improved, with reduced upper lip retrusion and lower lip protrusion as a result of the maxillary advancement and mandibular setback, respectively. Although gingival recession showed a slight increase, tooth mobility was within the normal physiological range. No tooth hyperesthesia was observed after treatment. There was negligible osseous relapse, and the occlusion remained stable after 5 years of post-treatment retention. Our findings suggest that such multidisciplinary approaches for the treatment of CLP with gingival recession and occlusal collapse help in improving occlusion and facial esthetics without the need for prostheses such as dental implants or bridges; in addition, the results show long-term post-treatment stability.

• 천문학회보
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• 제40권1호
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• pp.68.1-68.1
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• 2015

Gravitational collapse is a dynamical process associated with star formation. One observational evidence of such infall motion is so called "blue asymmetry" profile, which is the optically thick line profile with the intensity peak skewed blueward relative to the intensity peak of optically thin lines. We analyzed both HCN J=1-0 and HNC J=1-0 line profiles to study the inflow motion in different evolutionary stages of massive star formation; Infrared dark clouds (IRDCs), High-mass protostellar object (HMPOs), and Ultra-compact HII regions (UCHIIs). The infall asymmetry in the HCN spectra seems to be more prevalent than the HNC spectra throughout all the three evolutionary phases. The prevalence of the blue profile in the HCN spectra is found in every evolutionary stage, with IRDCs showing the largest blue excess. In the case of the HNC spectra, only IRDCs show the blue excess statistically significant. These results suggest that HCN may be a better infall tracer in massive star forming region. In addition, even though the characteristics of the blue profile largely depend on the suitable combination of optical depth and critical density, our analyses also indicate that IRDCs may have the most active infall process compared to other evolutionary phases.