• 제목/요약/키워드: Large Field Density Test

검색결과 42건 처리시간 0.026초

현장밀도시험을 이용한 암성토 체적환산계수 산정에 관한 연구 (The Estimation of Volume Conversion Factor of Rock Fill using Field Density Test)

  • 박종범;마명수
    • 한국지반신소재학회논문집
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    • 제16권1호
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    • pp.9-17
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    • 2017
  • 본 연구에서는 암성토의 토공량 설계에 대한 대책방안으로 현장밀도시험을 수행하였으며, 현장밀도시험결과 암성토부의 발파암 평균 체적환산계수는 1.001로서 풍화암의 체적환산계수 1.1보다 작은 값이 나타났다. 이와 같이 암성토의 경우 여러 가지 현상에 의해 토공량의 증감 원인을 제공하고 있으나, 이에 대한 조사 및 시험방법 등 구체적인 기술 등이 부족한 실정이므로 본 연구결과에서와 같이 체적환산계수를 검토하기 위한 조사방법으로 현장밀도시험방법이 매우 유용한 방법임을 확인하였다.

대형다짐시험 및 표준다짐시험을 이용한 파쇄암 성토재의 다짐특성 연구 (The Study of Compaction Characteristics of Cataclasite Fill Material using Large and Standard Compaction Tests)

  • 정재형;류상훈;최동엽;박광식;황성필
    • 지질공학
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    • 제26권4호
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    • pp.439-445
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    • 2016
  • 신축되는 공항은 미래 항공수요를 선점하고 주변지역 공항들과의 경쟁에서 앞서나가기 위해, 고품질의 활주로를 건설하고자 체계적으로 활주로 하부지반 건설에 임하고 있다. 본 연구에서는 여객계류장 운영시 하부 연약지반의 잔류침하를 최소화 할 수 있도록 시공관리하기 위하여 기존의 표준다짐시험의 단점을 보완하는 연구를 하고자 하였으며, 직경 100 mm 이하의 성토 재료를 사용한 4개소 현장에서 성토재료를 채취하여 표준다짐시험(KS F 2312), 대형원형몰드 다짐시험, 물치환 현장밀도시험(ASTM D 5030)을 수행하였다. 현장밀도시험과 표준 실내다짐시험의 상관관계를 회귀분석 하면, 유의수준(P-value) 0.05에서 신뢰할 수 없는 값을 나타내었으며, 현장밀도시험과 대형 실내다짐시험의 회귀분석 결과 상관계수(R)가 0.8878로 상관관계가 높게 나타났다. 설계 및 시공에 사용되는 최대건조밀도를 평가할 때 성토재료의 최대치수를 고려하여 다짐시험방법이 선택되어야만 현장여건이 충실히 반영되어 전체적으로 균질한 품질의 시공이 이루어 질 수 있을 것으로 판단된다.

대형전단시험을 통한 댐제체용 조립재료의 경험적 설계정수에 대한 평가 (Evaluation of Empirical Design Factors of Coarse Grained Material through Large Scale Shear Test)

  • 오기대;김경열;이대수
    • 한국지반공학회:학술대회논문집
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    • 한국지반공학회 2006년도 춘계 학술발표회 논문집
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    • pp.777-783
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    • 2006
  • The coarse grained materials are used in various construction field such as express way back fill, Dam etc. Especially, for dam construction, a huge mount of rock fill materials are needed, so around domestic stony mountains are generally developed to produce materials. Not an accurate theory, but design criteria is based on empirical factors that were constructed in advance for design of dam especially Concrete Face Rockfill Dam(CFRD). Considering the post facts, the modified design criteria are essential in the future with more theoretical and experimental ways. In this study, large scale direct shear tests are performed with various relative density conditions on coarse grained material of Yecheon area to compare test results and general CFRD design factors.

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Conceptual design and fabrication test of the HTS magnets for a 500 W-class superconducting DC rotating machine under 77 K

  • Choi, J.;Kim, S.K.
    • 한국초전도ㆍ저온공학회논문지
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    • 제23권4호
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    • pp.35-38
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    • 2021
  • Conventional direct current (DC) rotating machines are usually used for crane and press machine using high torque in metal and steel industries, because of a constant output power along variable rotating speed. A general DC motor with permanent field magnets could not increase a magnetic flux density at a gap between armature coils and field magnets. However, a superconducting DC motor has field magnets composed with high temperature superconducting (HTS) coils and it could increase the magnetic flux density at the gap to over 10 times than those of a general DC motor by control the excitation current into HTS coils. The superconducting DC motor could be operated with extremely high torque and constant output power at a low rotational speed. In this paper, a 500 W superconducting DC rotating machine was conceptually designed with a LN2 (Liquid Nitrogen) cooling method and the operation characteristics results of HTS field magnets were presented. The two no-insulation HTS magnets for a 500 W superconducting DC rotating machine were fabricated. The excitation current for the HTS magnets could be controlled from 0 to 40 A. This test results will be available to design large-sized HTS magnets for a number of hundred kW class superconducting DC rotating machine under LN2 cooling system.

Applying Alcock-Paczynski Test to the Large Scale Structure

  • Li, Xiao-Dong;Park, Changborm;Romero, Jaime Forero
    • 천문학회보
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    • 제38권2호
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    • pp.58.1-58.1
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    • 2013
  • The main idea of the Alcock-Paczynski (AP) test is that, if we use a wrong distance-redshift relation to infer the shape of a spherical object in the Universe, this object may look non-spherical. To probe the cosmic expansion history through the AP test, the key point is to find something which is known as spherical in the Universe. We propose two possible ways applying the AP test to the large scale structure (LSS): 1) Based on the observed galaxies or quasars, one built up the beta-skeleton tracing the LSS, and investigating the inhomogeneity of the connections; 2) One reconstructs the smoothed density-contrast gradient field based on LSS observations, and investigating the inhomogeneity of the gradient vectors. Compared with some existed methods probing AP effect through 2-point correlation function, galaxy pairs, or voids, our methods have various advantages: 1) The information of both the high and low dense regions of the LSS are taken into account. 2) The redshift space distortion as the main contamination to the AP effect can be easily removed.

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전류 밀도가 다른 선재들의 자화손실 특성 평가 (Estimation of Magnetization loss of HTS wires with Different Current Density)

  • 임형우;윤기현;이희준;차귀수
    • 한국초전도ㆍ저온공학회논문지
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    • 제9권1호
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    • pp.72-75
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    • 2007
  • Magnetization loss of HTS wire is strongly dependent on the critical current density and the aspect ration of the HTS wire. This paper presents the magnetization loss of stacked BSCCO wire and stacked YBCO wires which had different critical current densities. Width of the BSCCO wire was 4mm and widths of two YBCO wires were 4mm and 8mm. Single wire, two stacked three stacked and four stacked wires were fabricated and tested. Ratio of magnetization loss of BSCCO wire to YBCO wire was presented at single wire. For stacked wire, ratio of magnetization loss of single wire to stacked wire was presented. Test results shows that magnetization losses of stacked wires were greater than that of single wire at large high magnetic field above critical magnetic field.

Uniform large scale cohesionless soil sample preparation using mobile pluviator

  • Jamil, Irfan;Ahmad, Irshad;Ullah, Wali;Junaid, Muhammad;Khan, Shahid Ali
    • Geomechanics and Engineering
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    • 제28권5호
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    • pp.521-529
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    • 2022
  • This research work deals with the development of air pluviation method for preparing uniform sand specimens for conducting large scale laboratory testing. Simulating real field conditions and to get reliable results, air pluviation method is highly desirable. This paper presents a special technique called air pluviation or sand raining technique for achieving uniform relative density. The apparatus is accompanied by a hopper, shutters with different orifice sizes and numbers and set of sieves. Before using this apparatus, calibration curves are drawn for relative density against different height of fall (H) and shutter sizes. From these calibration curves, corresponding to the desired relative density of 60%, the shutter size of 13mm and height of fall of 457.2 mm, are selected and maintained throughout the pluviation process. The density obtained from the mobile pluviator is then verified using the Dynamic Cone Penetrometer (DCP) test where the soil is poured in the box using defined shutter size and fall height. The results obtained from the DCP test are averaged as 60±0.5 which was desirable. The mobile pluviator used in this research is also capable of obtaining relative densities up to 90%. The instrument is validated using experimental and numerical approach. In numerical study, Plaxis 3D software is used in which the soil mass is defined by 10-Node tetrahedral elements and 6-Node plate is used to simulate plate behavior in the validation phase. The results obtained from numerical approach were compared with that of experimental one which showed very close correlation.

Critical Characteristics Estimation of a Large-Scale HTS Wind Turbine Generator Using a Performance Evaluation System

  • Kim, Taewon;Woo, Sang-Kyun;Kim, Changhyun
    • KEPCO Journal on Electric Power and Energy
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    • 제5권3호
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    • pp.229-233
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    • 2019
  • Large-scale High Temperature Superconducting (HTS) wind power generators suffer from high electromagnetic force and high torque due to their high current density and low rotational speed. Therefore, the torque and Lorentz force of HTS wind power generators should be carefully investigated. In this paper, we proposed a Performance Evaluation System (PES) to physically test the structural stability of HTS coils with high torque before fabricating the generator. The PES is composed of the part of a pole-pair of the HTS generator for estimating the characteristic of the HTS coil. The 10 MW HTS generator and PES were analyzed using a 3D finite element method software. The performance of the HTS coil was evaluated by comparing the magnetic field distributions, the output power, and torque values of the 10 MW HTS generator and the PES. The magnetic flux densities, output power, and torque values of the HTS coils in the PES were the same as a pole-pair of the 10 MW HTS generator. Therefore, the PES-based evaluation method proposed in this paper can be used to estimate the critical characteristics of the HTS generator under high magnetic field and high torque before manufacturing the HTS wind turbines. These results will be used effectively to research and manufacture large-scale HTS wind turbine generators.

침식방지를 위한 토목섬유튜브의 거동 분석 (Behavior of Geotextile Tube for Erosion Control)

  • 장용채;손가영;이승은;김상진;김석우
    • 한국지반공학회논문집
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    • 제28권5호
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    • pp.5-12
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    • 2012
  • 토목섬유튜브공법은 고분자 합성섬유인 지오텍스타일을 활용하여 하천 및 해안구조물을 비롯하여 다양한 토목구조물을 축조할 수 있는 최신 적용공법이다. 본 논문에서는 해안가 모래의 침식을 방지를 위해 토목섬유튜브의 거동과 안정성, 침식방지 활용 가능성을 파악하고자 실내시험과 현장시험을 실시하였다. 실내시험인 대형직접전단시험 결과에 의하면 상대밀도가 증대됨에 따라 마찰각이 증가함을 알 수 있었고, 모래/토목섬유의 마찰각이 모래/모래의 마찰각보다 더 크게 나타났다. 현장시험 결과에 의하면 계측을 통해 시공 중 및 시공 후의 거동과 안정성을 파악하였고 침식방지 효과를 확인하였다.

Testing Web Feeding Model for Star Formation in Galaxy Clusters in the COSMOS Field

  • Ko, Eunhee;Im, Myungshin;Lee, Seong-Kook;Hyun, Minhee
    • 천문학회보
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    • 제46권1호
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    • pp.52.3-53
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    • 2021
  • It is yet to be understood what controls the star formation activity in high-redshift galaxy clusters. One recently proposed mechanism is that the star formation activity in galaxy clusters are fed by gas and galaxies in large-scale structures surrounding them, which we call as "web feeding model". Using galaxies in the COSMOS2015 catalog, with mass completeness at log(M/M⦿)≥9.54 and reliable photometric redshift data (σΔz/(1+z) ≲ 0.01), we study the star formation activities of galaxy clusters and their surrounding environment to test the web feeding model. We first identify the overdense regions with number density exceeding the 4σ-level from photometric redshift data as galaxy clusters, and we find that they are well matched with clusters identified in the X-ray extended source catalog. Furthermore, we identify galaxy large scale structures, and will present the correlation or anti-correlation between quiescent galaxy fraction, an indicator of star-forming activity, and the prevalence of galaxy large scale structures.

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