• Geomechanics and Engineering
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• 제36권1호
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• pp.51-69
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• 2024

Currently, composite lining mountain tunnels in China are generally classified based on the [BQ] method for the surrounding rock grade. Increasingly, tunnel field construction is replicated indoors for scale down model tests. However, the development of analogous materials for model tests of composite lining tunnels with different surrounding rock grades is still unclear. In this study, typical Class III and V surrounding rock analogous materials and corresponding composite lining support materials were developed. The whole processes of excavation-support dynamics of the mountain tunnels were simulated. Data on the variation of deformations, contact pressures and strains on the surrounding rock were obtained. Finally, a comparative analysis between model tests and numerical simulations was performed to verify the rationality of analogous material development. The following useful conclusions were obtained by analyzing the data from the tests. The main analogous materials of Class III surrounding rock are barite powder, high-strength gypsum and quartz sand with fly ash, quartz sand, anhydrous ethanol and rosin for Class V surrounding rock. Analogous materials for rockbolts, steel arches are replaced by aluminum bar and iron bar respectively with both shotcrete and secondary lining corresponding to gypsum and water. In addition, load release rate of Class V surrounding rock should be less than Class III surrounding rock. The fenestration level had large influence on the load sharing ratio of the secondary lining, with a difference of more than 30%, while the influence of the support time was smaller. The Sharing ratios of secondary lining in Class III surrounding rock do not exceed 12%, while those of Class V surrounding rock exceed 40%. The overall difference between the results of model tests and numerical simulations is small, which verifies the feasibility of similar material development in this study.

• 자원환경지질
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• 제7권3호
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• pp.101-122
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• 1974

The study area is located in between Susanri and Hwanggangri where the formations of Okcheon group and Chosun group supposedly come in contact so that the area is structurally very import. Present study reveals that the meta-volcanic rocks distribute from south to north along contact zone of Okcheon and Chosun groups in the center of the area. Meta-volcanic rocks seem to be originated from the andesite or andesitic basalt rocks which was known to be Surchangri formation consist of phyllite and black slate by previous workers. The meta-volcanic rocks intruded along the fault zone one existed between Okcheon and Chosun groups but obliterated at present by the intrusion of volcanic rocks. The fault seems to be overthrust, and one of the positive evidences of thrust fault is the Yamisan nappe structure in Yamisan near Susanri. This interpretation coincides with O.J. Kim's work which states that the Precambrian Okcheon group is largely overturned and thrusted over the Chosun group. The relation between the Surchangri and the Majeonri formation marks facies change. This fact together with northpluging anticlinal structure made it possible that both formation came into contact along direction without fault. Yongam formation is not overlain unconformably used to be believed by previous workers, but interbed in the Great Limestone series of Chosun goup. It is also clarified that the rock formerly designated as limesilicate rock was meta-liparite. The origin of amphibole pebbles in the Kunjasan formation is of primary and secondary ones; the secondary pebbles were formed by metamorphism of the fragments of limestone or dolomite.

• 천문학회지
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• 제39권2호
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• pp.41-50
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• 2006

We present the results of new multi-color CCD photometry for the contact binary XZ Leo, together with reasonable explanations for the period and light variations. Six new times of minimum light have been determined. A period study with all available timings confirms Qian's (2001) finding that the O-C residuals have varied secularly according to $dP/dt\;=\;+8.20{\times}10^{-8}\;d\;yr^{-l}$. This trend could be interpreted as a conservative mass transfer from the less massive cool secondary to the more massive hot primary in the system with a mass flow rate of about $5.37{\times}10^{-8}\;M_{\odot}\;yr^{-l}$. By simultaneous analysis of our light curves and the previously published radial-velocity data, a consistent set of light and velocity parameters for XZ Leo is obtained. The small differences between the observed and theoretical light curves are modelled by a blue third light and by a hot spot near the neck of the primary component. Our period study does not support the tertiary light but the hot region which may be formed by gas streams from the cool secondary. The solution indicates that XZ Leo is a deep contact binary with the values of q=0.343, $i=78^{\circ}.8$, ${\Delta}(T_1-T_2)=126\;K$, and f=33.6 %, differing much from those of Niarchos et al. (1994). Absolute parameters of XZ Leo are determined as follows: $M_1=1.84\;M_{\odot},\;M_2=0.63\;M_{\odot},\;R_1=1.75\;R_{\odot},\;R_2=1.10\;R_{\odot},\;L_1=7.19\;L_{\odot},\;and\;L_2=2.66\;L_{\odot}$.

• 대한한의학방제학회지
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• 제8권1호
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• pp.257-279
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• 2000

Allergic contact dermatitis is a common skin disease resulting from specific immunologic to topically applied various allergen. After Dinitrochlorobenzene (DNCB) secondary sensitization, the ICR mice administered Rhemanniae radix extract (RRE) was observed to ascerstain the effect of RRE on allergic contact dermatitis. Purpose of this study was to investigate contact hypersensitivity assay, abdominal skin morphologic changes. Including mast cells and cell-surface glycoconjugates. The change of interleukin 2 (IL-2) receptor (CD25R). ICAM in abdominal skin, lymph node of inguinal region, and electro microscope-morphologic changes of abdominal skin. The results of this study were as follows: 1. The contact hypersensitivity assay, the ear swelling in the RRE had lesser probability than in the ACD Group. 2. In the general morphologic change of skin, hyperplasia of keratinocytes, distribution of vasculogenesis and epidermal lymphocytes infiltration were decreased in the RRE group compared with the ACD group. In epidermal basal layer and prickle layer, cell damage was decreased in the RRE group compared with the group painted with ACD. 3. MasT-cell in dermis was decreased in the RRE group compared with the group painted with DNCB. 4. Distribution of interlukin-2 Receptior positive cell and ICAM positive cell in dermis was decreased in the RRE Group compared with the ACD group. 5. Distribution of helper T-lymphocyte and cytotoxic T-lymphocite in inguinal nodes was decreased in the RRE group, and was observed well in paracortical area and cortical cord. 6. Distribution of apoptotic cell was appeared in the RRE group compared with the ACD group, in skin, dermis. in inguinal nodes, paracortical area observed well. With above results, the restarint of immunosuppression occuring in Allergic contact dermatitis is resulted in the slow progress the effect of Allergic contact dermatitis, and it is thought that ithis fact has a series of relation with apoptosis.

• 한국사회복지학
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• 제68권1호
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• pp.117-140
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• 2016

이 연구의 목적은 성폭력 피해 아동 청소년이 인지하는 2차 피해의 경험을 보다 깊이 있게 탐색하는 것이다. 연구 목적을 달성하기 위해 2차 피해 경험이 있다고 스스로 인지하고 있는 성폭력 피해 아동 청소년 6명을 연구참여자로 섭외하였고, 2~4회에 걸친 심층면접을 통해 자료를 수집하였다. 수집된 자료는 Colaizzi가 제시한 분석 방법에 따라 분석하였다. 분석 결과 '상처 위에 소금 뿌리는 가해자', '비빌 언덕조차 되어주지 않는 가족', '울타리가 무너진 학교', '상처를 덧내는 사법기관', '믿었던 도끼로 발등 찍는 상담원', '강 건너 불구경하는 이웃'이라는 6개 하위범주를 도출할 수 있었다. 아동 청소년이 경험하는 2차 피해는 성폭력이라는 1차 피해 후에 '이중삼중으로 밀려오는 후폭풍'과 같은 경험으로 드러났다. 연구 결과를 토대로 아동 청소년 성폭력 2차 피해 예방을 위한 사회복지적 함의에 대해 논의하였다.

• 전력전자학회논문지
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• 제11권3호
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• pp.216-223
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• 2006

태양광 발전 시스템을 위한 무접점 변압기 적용 고효율 Full-bridge LLC 공진컨버터를 제안하였다. 제안된 LLC 공진컨버터는 직렬 커패시터와의 직렬공진을 위해 무접점 변압기의 누설인덕턴스와 자화인덕턴스를 이용하였다. 제안된 LLC 공진컨버터는 공진주파수 보다 높은 스위칭영역에서 연속 공진전류로 동작하는 기존 직렬공진 컨버터와는 달리 공진주파수 아래의 좁은 주파수 범위에서 불연속 공진전류로 동작한다. 이러한 불연속모드 공진전류 때문에 제안된 컨버터는 어떤 보조회로 없이 무접점 변압기 1차측 주스위칭 소자의 영 전압 스위칭(ZVS)과 2차측 다이오드의 영 전류 스위칭(ZCS)을 얻을 수 있고, 높은 전압이득특성을 갖는다. 본 논문에서는 무접점 변압기 적용 Full-bridge LLC 공진컨버터를 이용한 무접점 전원장치에 대한 이론적 해석 및 시뮬레이션을 통해 150W급 시제품을 제작하여 태양광 발전 전원시스템에 적용 실험한 결과를 서술했다.

• Structural Engineering and Mechanics
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• 제76권2호
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• pp.153-162
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• 2020

Aiming at the mechanical and structural characteristics of the contact zone composite rock, the shear tests and numerical studies were carried out. The effects of the differences in mechanical properties of different materials and the normal stress on shear properties of contact zone composite samples were analyzed from a macro-meso level. The results show that the composite samples have high shear strength, and the interface of different materials has strong adhesion. The differences in mechanical properties of materials weakens the shear strength and increase the shear brittleness of the sample, while normal stress will inhibit these effect. Under low/high normal stress, the sample show two failure modes, at the meso-damage level: elastic-shearing-frictional sliding and elastic-extrusion wear. This is mainly controlled by the contact and friction state of the material after damage. The secondary failure of undulating structure under normal-shear stress is the nature of extrusion wear, which is positively correlated to the normal stress and the degree of difference in mechanical properties of different materials. The increase of the mechanical difference of the sample will enhance the shear brittleness under lower normal stress and the shear interaction under higher normal stress.

• Journal of Astronomy and Space Sciences
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• 제22권3호
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• pp.223-232
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• 2005

질량비가 작은 접촉쌍성 V410 Aur과V776 Cas를 소백산천문대의 61cm망원경에 2K CCD 카메라를 부착하여 측광 관측을 하였으며, 그 결과 이 별들의 새로운 3색(BVR)의 완전한 광도곡선을 얻었다. 새로운 광도곡선과 이미 발표된 분광관측으로부터 WD모델을 이용하여 이 두 별의 궤도요소와 절대 물리량을 얻었다. V410 Aur과 V776 Cas를 포함한 절대물리량이 잘 알려진 19개의 질량비가 작은 접촉쌍성들의 진화 상태를 조사하였다. 그 결과 질량비가 작은 접촉쌍성의 주성은 대부분 TAMS상에 놓이며 반성은 ZAMS 아래 놓이고 있음을 재확인하였다.

• Journal of Astronomy and Space Sciences
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• 제23권3호
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• pp.189-198
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• 2006

BVRI CCD 측광 관측에 의하여 질량비가 작은 접촉쌍성 HN UMa와 II UMa의 새로운 광도곡선을 얻었다. 새로운 광도곡선과 이미 발표된 분광관측으로부터 Wilson-Devinney 프로그램을 이용하여 이 두 별의 궤도요소와 절대 물리량을 얻었다. HN UMa와 II UMa를 포함한 절대물리량이 잘 알려진 21개의 질량비가 작은 접촉쌍성들의 진화 상태를 조사하였다. 그 결과 질랑비가 작은 접촉쌍성의 반성은 영년주계열 아래 놓이며, 이러한 현상은 질량이 작은 접촉쌍성의 반성에서의 질량손실을 가정할 경우, 비록 작의 양의 질량이지만 반성에서의 질량 감소는 상대적으로 광도의 감소가 현저히 작아지기 때문일 것으로 예상된다.

• Journal of Astronomy and Space Sciences
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• 제16권2호
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• pp.227-240
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• 1999

소백산천문대의 61cm 망원경을 이용하여 1996년 5월 12일과 1999년 5월 5일부터 6월 8일까지 총 8일 밤 동안 W UMa 형 접촉쌍성 BV Dra의 CCD 측광광측을 수행하여 이 쌍성계의 BV R광도 곡선을 완성하였다. 우리의 관측으로부터 9개의 새로운 극심시간 (제1 극심: 5개, 제2 극심: 4개)을 산출하였고, 1999년 이후에 관측된 극심시간으로부터 새로운 광도요소를 결정하였다. 우리의 BV R광도곡선과 Batten & Lu (1986)의 시선속도곡선을 Wilson-Devinney 쌍성모델의 접촉모드 (Mode 3)에 적용하여 BV Dra의 측광 및 분광학적 해를 구하였다. 이 분석에서 광도곡선 비대칭의 원인을 흑점에 의한 것으로 가정하여 흑점이 있는 경우와 없는 경우로 나누어 1999년 광도곡선 해를 산출하였다. 그 결과, 우리는 이전의 연구자들에 의해 보고되지 않은 광도곡선 비대칭을 반성표면 위에 hot spot가 존재하고, 주성표면 위에 cool spot가 존재해서 일어난다고 해석하였다. 광도곡선과 시선속도곡선의 분석에 의해 산출한 BV Dra의 절대 물리량은 $M_1=0.40M_{odot}$, $M_2=1.01M_{odot}$, $R_1=0.72R_{odot}$, $R_2=0.40R_{odot}$ 이다. 이 절대 물리량을 이용하여 질량-반경도를 살펴본 결과, 질량이 작은 주성이 종년 주계열 (TAMS)근처에 있고, 질량이 큰 반성이 영년주계열 (ZAMS)근처에 위치하고 있다. 이는 질량-반경도에서 다른 W형 W UMa쌍성계의 위치와 매우 비슷하다.