• 지질공학
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• 제24권4호
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• pp.525-534
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• 2014

폐광 부지에서 발생하는 대표적인 환경 문제는 산성으로 오염된 지표수와 지하수, 적재된 폐광석 및 광미, 채굴 활동으로 야기된 지반침하 현상을 들 수 있다. 이 논문은 광해 유형에 따라 재해 및 오염영역을 효율적으로 탐지했던 지구물리탐사방법들을 고찰하는데 있다. 시험 자료로서 토양오염, 산성광산배수, 지반침하, 인공차수막 파손 및 광미/폐광석 적치장을 각각 대표하는 네 개의 폐광 부지를 선택하였다. 자료 검증을 위해 물리탐사자료는 자료의 유형에 따라 시추자료(코어 샘플, 물리검층, 토모그래피 등)와 물 자료(수소이온농도, 전기전도도, 중금속원소 등)와 비교하였다. 토양오염 탐지에 있어서 낮은 전기비저항 이상대는 특히 구리, 납, 아연의 중금속 농도가 높은 지역과 부합된다. 산성광산배수의 유동 경로는 자연전위 곡선에서 음의 전위 이상대, 전기비저항자료에서의 저비저항 이상대, 지하레이더 자료에서의 얕은 투과깊이 영역으로 탐지되었다. 채굴적은 전기비저항 단면에서의 저비저항 이상대, 탄성파토모그래피에서 낮은 속도 영역, 물리검층곡선의 복합해석으로 특징되며, 정확한 위치는 코어자료와 시추공영상자료에서 잘 확인되었다. 침출수 유동을 차단하기 위해 설치된 인공차수막의 파손 구간은 전기비저항 자료에서의 국부적인 이상대로 정확히 탐지되며 매립된 폐석더미는 고비저항 이상대와 저속도 이상대로 특징된다.

• 지구물리와물리탐사
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• 제9권3호
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• pp.241-249
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• 2006

한국의 지질 환경은 암석 분포가 매우 다양하고 복잡한 구조 활동의 영향을 받아 지하매질의 이방성 특성이 국부적으로 심하게 변화한다. 기존의 이방성 주시 모델링의 경우 지질 모델을 2차원으로 단순화시킴으로써 이러한 복잡한 지질 환경을 제대로 고려할 수 없었다. 또한 약 이방성 가정을 사용하여 실제로 나타날 수 있는 지하 매질의 심각한 이방성 영향을 주시 모델링에서 고려할 수 없었다. 이에 이 연구에서는 보다 실제적이고 복잡한 3차원 횡등방성 매질(transversely isotropic media)에서 q-P파의 초동 주시 양상을 모사할 수 있는 주시 모델링 알고리듬을 개발하였다. 이 알고리듬에서는 2차원 비선형 주시 내삽(2D nonlinear traveltime interpolation) 기법과 주시의 3차원 격자 채움법(mapping)을 이용한 직접 전파법(direct calculation)을 통해 급격한 물성의 변화에도 주시 계산이 가능하도록 하였다. 또한, 최소 주시 계산과정에서 수치 미분을 통한 최대 경사법(steepest descent method)을 사용하여 약 이방성 가정을 극복하였다. 개발된 알고리듬은 해석해와 비교하여 그 타당성을 검증하였고 3차원 2층구조에 대한 주시 계산을 수행하여 물성이 급격히 변화하는 모델에 대해서도 안정적으로 주시 계산이 이루어짐을 확인하였다. 이 연구에서 개발한 3차원 주시 모델링 알고리듬은 향후 구조보정이나 토모그래피 알고리듬 개발에 사용될 수 있을 것으로 기대한다.

• Journal of Mechanical Science and Technology
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• 제14권3호
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• pp.320-330
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• 2000

It is desirable to perform nondestructive evaluation (NDE) to assess material properties and part homogeneity because the manufacturing of carbon/carbon brake disks requires complicated and costly processes. In this work several ultrasonic techniques were applied to carbon/carbon brake disks (322mm ad, 135mm id) for the evaluation of spatial variations in material properties that are attributable to the manufacturing process. In a large carbon/carbon disk manufactured by chemical vapor infiltration (CYI) method, the spatial variation of ultrasonic velocity was measured and found to be consistent with the densification behavior in CYI process. Low frequency (e.g., 1-5MHz) through-transmission scans based on both amplitude and time-of-flight of the ultrasonic pulse were used for mapping out the material property inhomogeneity. Images based on both the amplitude and the time-of-flight of the transmitted ultrasonic pulse showed significant variation in the radial direction. The radial variations in ultrasonic velocity and attenuation were attributed to a density variation caused by the more efficient densification of pitch impregnation near the id and od and by the less efficient densification away from the exposed edged of the disk. Ultrasonic velocities in the edges of the disk. Ultrasonic velocities in the thickness direction were also measured as a function of location using dry-coupling transducers ; the results were consistent with the densification behavior. However, velocities in the in-plane directions (circumferential and radial) seemed to be affected more by the relative contents of fabric and chopped fiber, and less by the void content.

• 터널과지하공간
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• 제2권2호
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• pp.212-223
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• 1992

The distinct element method(DEM) si well suited to the kinematic analysis of blocky rock masses. Two distinctive problems, a rock avalache and tunnel in jointed rock masses, are chosen to apply the DEM which is based on perfectly rigid behaviour of blocks. Investigated for both problems are the effects of the input parameters such as contact stiffnesses, friction coefficient and damping property. Using various types of models of the avalanche and tunne, an extensive parametric study is done to gain experiences in the method, and then to alleviate difficulties in determining parameter values suitable for a given problem. The coefficient of frictio has significant effects on all aspects of avalanche motion(travel distance, velocity and travel time), while the stiffnesses affect the rebounding and jumping motions after collision. The motion predicted by the models having single and mutiple blocks agrees well to the observations reported on the actual avalache. For the tunnel problem, the behaviour of the key block in an example tunnel is compared by testing values of the input parameters. The stability of the tunnel is dependent primarily on the friction coefficient, while the stiffness and damping properties influence the block velocity. The kinematic stability of a tunnel for underground unclear waste repository is analyzed using the joint geometry data(orientation, spacing and persistence) occurred in a tailrace tunnel. Allowing a small deviation to the mean orientation results in different modes of failure of the rock blocks around the tunnel. Of all parameters tested, the most important to the stability of the tunnel in blocky rock masses are the geometry of the blocks generated by mapping the joint and tunnel surfaces in 3-dimensions and also the friction coefficient of the joints particularly for the stability of the side walls.

• 천문학회보
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• 제43권1호
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• pp.66.1-66.1
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• 2018

Turbulence is a phenomenon which largely determines the density and velocity fields in molecular clouds. Turbulence can produce density fluctuation which triggers a gravitational collapse, and it can also produce a non-thermal pressure against gravity. Therefore, turbulence controls the mode and tempo of star formation. However, despite many years of study, the properties of turbulence remain poorly understood. As part of the Taeduk Radio Astronomy Observatory (TRAO) Key Science Program (KSP), "apping Turbulent properties In star-forming MolEcular clouds down to the Sonic scale (TIMES; PI: Jeong-Eun Lee)", we have mapped two star-forming clouds, the Orion A and the ${\rho}$ Ophiuchus molecular clouds, in 3 sets of lines (13CO 1-0/C18O 1-0, HCN 1-0/HCO+ 1-0, and CS 2-1/N2H+ 1-0) using the TRAO 14-m telescope. We aim to map entire clouds with a high-velocity resolution (~0.05 km/s) to compare turbulent properties between two different star-forming environments. We will present the preliminary results using a statistical method, Principal Component Analysis (PCA), that is a useful tool to represent turbulent power spectrum.

• 천문학회보
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• 제44권2호
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• pp.68.1-68.1
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• 2019

Turbulence plays a crucial role in controlling star formation as it produces density fluctuation as well as non-thermal pressure against gravity. Therefore, turbulence controls the mode and tempo of star formation. However, despite a plenty of previous studies, the properties of turbulence remain poorly understood. As part of the Taeduk Radio Astronomy Observatory (TRAO) Key Science Program (KSP), "mapping Turbulent properties In star-forming MolEcular clouds down to the Sonic scale (TIMES; PI: Jeong-Eun Lee)", we mapped the Orion A and the Ophiuchus clouds, in three sets of lines (13CO 1-0/C18O 1-0, HCN 1-0/HCO+ 1-0, and CS 2-1/N2H+ 1-0) with a high-velocity resolution (~0.1 km/s) using the TRAO 14-m telescope. The mean Trms for the observed maps are less than 0.25 K, and all these maps show uniform Trms values throughout the observed area. These homogeneous and high signal-to-noise ratio data provide the best chance to probe the nature of turbulence in two different star-forming clouds, the Orion A and Ophiuchus clouds. We present comparisons between the line intensities of different molecular tracers as well as the results of a Principal Component Analysis (PCA).

• Korean Circulation Journal
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• 제52권5호
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• pp.368-378
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• 2022

Background and Objectives: Recurrence rates after radiofrequency catheter ablation (RFCA) in atrial fibrillation (AF) patients are not low especially in non-paroxysmal AF. The diameter of left atrium (LA) has been widely used to predict the recurrence after RFCA for decades. However, LA diameter represents structural remodeling of LA and does not reflect electrical remodeling. We aimed to determine the predictive value of electrical remodeling of LA which is represented by the amount of low voltage zone (LVZ). Methods: We performed a retrospective cohort analysis of AF patients who underwent de novo RFCA in a single-center. Results: A total of 3,120 AF patients with de novo RFCA were analyzed. Among these patients, 537 patients underwent an electroanatomic mapping with bipolar voltage measurement of LA. The diameter of LA and flow velocity of LA appendage (LAA) differed significantly according to quartile group of LVZ area and percentage: patients with high LVZ had large LA diameter and low LAA flow velocity (p<0.001). Freedom from late recurrence (LR) was significantly lower in patients with high LVZ area and percentage (p<0.001). The diameter and surface area of LA had area under curve (AUC) of 0.592 and 0.593, respectively (p=0.002 for both). The predictive value of LVZ area (AUC, 0.676) and percentage (AUC, 0.671) were both superior compared with LA diameter (p=0.011 and 0.027 for each comparison). Conclusions: In conclusion, LVZ can predict freedom from LR after RFCA in AF patients. Predictive value was higher in parameters reflecting electrical rather than structural remodeling of LA.

• 한국신재생에너지학회:학술대회논문집
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• 한국신재생에너지학회 2007년도 춘계학술대회
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• pp.507-510
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• 2007

Piston cores retrieved from the western Ulleung Basin, East Sea were analyzed to examine the potential for hydrocarbon generation and to determine the hydrocarbon indicators. 2D multi-channel reflection seismic and Chirp data were also investigated for mapping and characterizing the geophysical hydrocarbon indicators such as BSR (bottom simulating reflector), blank zone, pock-mark etc. High organic carbon contents and sedimentation rates that suggest good condition for hydrocarbon generation. High pressure and low temperature condition, and high residual hydrocarbon concentrations are favor the formation of natural gas hydrate. In the piston cores, cracks generally oriented to bedding may indicate the gas expansion. The seismic data show several BSRs that are associated with natural gas hydrates and underlying free gas. A number of vertical to sub-vertical blank zones were well identified in the seismic sections. They often show the seismic pull-up structures, probably indicating the presence of high velocity hydrates. Numerous pockmarks were also observed in the Chirp profiles. They may indicate the presence of free gas below the hydrate stability zone as well.

• 한국소음진동공학회:학술대회논문집
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• 한국소음진동공학회 2007년도 춘계학술대회논문집
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• pp.628-632
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• 2007

The purpose of study is to confirm a acceptable range of data errors in data collecting. To examine a acceptable range of data errors, emission level is calculated for a vehicle flow and heavy vehicle percentage as a function of small-sized velocity. According to road selected, noise level of detail influence road noise calculations. It can be concluded that a vehicle flow raised an error less than 5000(veh/h) for a maximum error in emission level of 3.01dB, and the more a heavy vehicle percentage have a low value, the more emission level is a slight difference. This analysis gives insight regarding the accuracy of traffic flow data that is needed to reach a certain level of accuracy for the resulting noise level.

• 한국항공우주학회지
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• 제34권5호
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• pp.74-80
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• 2006

1980년대부터 민간에 개방된 GPS는 C/A코드의 도달시간을 측정하여 위치를 계산하고, 반송파의 도플러 주파수를 측정하여 속도를 계산한다. 위치정확도를 향상시키기 위하여 공통오차를 제거하는 DGPS 기법과 반송파 위상을 이용하여 수cm 내의 정확도를 가질 수 있는 CDGPS 기법이 1990년대부터 개발되기 시작하였다. 본 논문에서는 CDGPS를 위해 LSAST 미지정수 추정기법을 개선하여 계산효율 및 신뢰도를 높이고, 단일 주파수 GPS 수신기를 이용하여 움직이는 항체의 상대위치를 수cm 내의 정확도로 측정한 실험결과를 INS의 위치와 비교하여 제시한다. 이러한 결과는 추후 정밀관성항법장치, 무인자율주행, 측지 및 정밀지도제작 등에 유용하게 쓰일 수 있다.