• 융합정보논문지
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• 제10권10호
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• pp.196-202
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• 2020

본 연구는 경영학에 대한 대학생들의 학습개념을 알아보고 학습개념이 학습접근과 비판적 사고에 미치는 영향을 알아보았다. 편의 표집한 경영학 전공/부전공 학생들을 대상으로 온라인 설문을 실시하였다. 총 88명의 응답 분석 결과, 경영학 전공/부전공 학생들에게 학습개념의 유의미한 성차 또는 학년차는 발견되지 않았다. '시험'과 '관점 확장' 학습개념이 심층적 접근에, '시험'이 표층적 접근에 유의미한 영향을 끼치는 것으로 나타났다. 또한, '관점 확장' 학습개념이 비판적 사고에 유의미한 영향을 미치는 것을 확인하였다. 이러한 연구결과는 고차원적 사고능력 향상을 목표로 수업 또는 교육과정 개선을 고민하는 교수자 또는 수업설계자들에게 좋은 지침 및 기초자료로 활용될 수 있을 것으로 기대된다.

• 한국지구물리탐사학회:학술대회논문집
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• 한국지구물리탐사학회 2005년도 공동학술대회 논문집
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• pp.55-58
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• 2005

CFRD (콘크리트 표면 차수벽형 석괴댐)에서 수행한 전기비저항 탐사 결과, 하부에서 매우 낮은 비저항대가 관측되었다. 일반적으로 CFRD 형식의 댐은 내부 포화가 발생하지 않는 것으로 알려져 있으나, 금번 조사에서 하부 20m 깊이에서 일정하게 저비저항대가 발견되어 이에 대한 검토를 위해 3차원 해석을 수행하였다. 탐사 당시의 수위는 댐 정상부에서 10m 정도 내려가 있는 상태였다. 첫 탐사 이후 6개월이 지난 후에 이루어진 탐사에서도 비슷한 양상을 보이고 있었다. 이에 대한 해석을 위해서 조사 댐의 모양을 대상으로 3차원 순산 모델링을 수행하고, 이에 대한 2차원 역산 해석을 적용하여 기존 해석 방법의 오류 가능성을 검토하였다. 또한 비저항 조사가 많이 적용된 중심코아 형 댐의 경우의 사례와 비교하였다. 해석 결과, 3차원 댐체 구조에 대한 2차원 역산 해석은 저수부의 수위와 밀접한 관련을 갖는 것으로 보이며, 3차원의 사다리꼴 기하구조로 인하여 댐 내부에 비저항의 이상대가 존재할 경우에도 그 민감도가 떨어지는 것으로 분석되었다.

• 천문학회보
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• 제41권2호
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• pp.49.2-49.2
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• 2016

The number of discovery of asteroids with peculiar rotational states has recently increased, and hence a novel approach for lightcurve analysis is considered to be critical. In order to investigate objects such as Non-Principal Axis (NPA) rotator, we selected a NPA candidate, (5247) Kryolv as our target considering its Principal Axis Rotation (PAR) code and the visibility in early 2016. The observations of Krylov were made using Korea Microlensing Telescope Network (KMTNet) 1.6 m telescopes installed at the three southern sites with TO (Target of Opportunity) observation mode. We conducted R-band time-series photometry over a total of 51 nights from January to April 2016 with several exposures during each allocated run. The ensemble normalization photometry was employed using the AAVSO Photomtric All-Sky Survey (APASS) catalog for the standardization. We successfully confirmed its NPA spin state based on the deviation from the reduced lightcurve, and thus Krylov is recorded as the first NPA rotator of its kind in the main-belt, with its precession and rotation periods, $P{\varphi}=81.18h$ and $P_{\Psi}=67.17h$, respectively. In this paper, we present the spin direction, the 3D shape model and taxonomy of the newly confirmed NPA asteroid (5247) Krylov.

• 한국항해항만학회:학술대회논문집
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• 한국항해항만학회 2005년도 춘계학술대회 논문집
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• pp.213-221
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• 2005

광양항은 부산항과 더불어 우리나라 컨테이너 화물 처리 Two Port System의 한축으로 개발 중인 동북아 중심항만(Hub Port)으로서 향후 2011년까지 총 33개의 컨테이너 선석 등이 개발 추진 중에 있어 해상교통량이 급격히 증가하고 있으며, 또한 거대선 ${\cdot}$ 위험화물운반선 ${\cdot}$ 고속여객선의 통항이 빈번하여 대형사고의 발생우려가 상존하고 있다. 본 연구에서는 광양항을 이용하는 선박의 입출항 항로 등에 대한 해상교통환경을 면밀히 분석${\cdot}$평가하고, 통항로 및 항행보조시설 등의 적정성 검토를 통하여 미래 지향적이고 안전한 해상교통환경을 조성하기 위한 체계적이고 종합적인 항로를 설정한다.

• 대한가정학회지
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• 제44권12호
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• pp.9-18
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• 2006

A case study was conducted on the development of patient clothes designs at the Korea University Medical Center, in order to provide an example of patient clothes designs which meet the hospital identity and the demands of patients and nurses. In this study, we focused on general patient pajamas and one-piece gowns worn in the obstetrics and gynecology department. A scientific and systematic design approach consisting of the following four steps was conducted in the designing process: needs assessment, design direction establishment, design presentation, and final decision. For the first step, focused group interviews and a survey were conducted to identify the needs of the patients and nurses. According to the results of the first step, 3 fabric patterns with light, modern, rhythmic, modest and ordinary images were designed utilizing the university and hospital symbols and logotypes. Fixed forms with realistic and geometric characteristics and colors, including white, yellow, blue, grey, and pink were selected to deliver the preferred image. Each fabric pattern was made in male and female versions of the color sets. The following styles of patient clothes were made with the 3 fabric samples: general patient pajamas with a U-neckline, 9/10-length sleeves and ankle-length pants, a full-length sleeved gown with openings for breast-feeding, and a gown with a deep back-neckline and button fastening. Different sizing systems for males and females were recommended for the production.

• 천문학회보
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• 제42권2호
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• pp.39.1-39.1
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• 2017

The standard hierarchical galaxy formation scenario in the popular LCDM cosmogony has been very successful in explaining the large-scale distribution of galaxies. However, one of the failures of the theory is that it predicts too many satellite galaxies associated with massive galaxies compared to observations, which is called the missing satellite galaxy problem. Isolated groups of galaxies hosted by passively evolving massive early-type galaxies are ideal laboratories for finding the missing physics in the current theory. We discover through a deep spectroscopic survey of galactic satellite systems that bright isolated early-type galaxies have almost no satellite galaxies fainter than the r-band absolute magnitude of about Mr=-14. The cutoff is at somewhat brighter magnitude of about Mr=-15 when only early-type satellites are used. Such a cutoff is not observed in the luminosity function of galaxies in the field. Physical properties of the observed satellites depend sensitively on the host-centric distance. All these are strong evidence that galactic satellites can become invisible due to astrophysics of satellite-host galaxy interaction. A recent state-of-the-art hydrodynamic simulation of galaxy formation does not reproduce such a cutoff in the satellite galaxy luminosity function. But the past history of the simulated satellites shows that many satellite galaxies near or somewhat fainter than the cutoff magnitude have recently become extinct through fatal encounters with the host or other satellite galaxies. Our observation indicates that the missing satellite galaxy problem could be mitigated if the astrophysics of galaxy interaction is more elaborated in the theory.

• 천문학회보
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• 제42권2호
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• pp.41.2-41.2
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• 2017

Discovered as the second highest S/N detection of the Planck SZ survey, PLCK G287.0+32.9 is a massive galaxy cluster that belongs to a rare collection of merging clusters that exhibit two radio relics and a radio halo. A feature that makes this cluster even more unique is the separation of the radio relics with one $\sim 400$ kpc to the north-west of the X-ray peak and the other $\sim 2.8$ Mpc to the south-east. This asymmetric configuration requires a complex merging scenario. A key to gaining insight into the events that caused the formation of the merging features is to understand the dark matter mass distribution. Using a weak-lensing technique on deep Subaru and Hubble Space Telescope observations, we map the dark matter mass distribution of PLCK G287.0+32.9. Our investigation detects five significant mass structures. The mass is dominated by a primary structure that is centered near the X-ray peak of the intracluster medium. Four lesser mass structures are detected with two located within $\sim 1\arcmin$ of the primary mass structure, a third to the north-west, and a fourth near the south-east radio relic. Along with these detections, we estimate the mass of each structure and relate their distributions to the intracluster medium and galaxy distributions. In addition, we discuss the relation of the mass structures to the formation of the relics and plausible merging scenarios.

• Ocean and Polar Research
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• 제31권2호
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• pp.167-176
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• 2009

Cobalt-rich manganese crusts on seamounts have received an increasing amount of attention as future resources for Co, Ni, Cu, and Mn. A dearth of detailed information regarding the relevant distribution characteristics, mining technologies, and ore processing technologies, however, has precluded potential evaluations of the technical and economic advantages of these crusts. In the past 4 years, Korea has undertaken a survey of the cobalt-rich manganese crusts in and around the Magellan Seamount and Mid-Pacific Mountains. This paper introduces the preliminary feasibility study of the distribution features and R&D results centered around the development of the cobalt-rich manganese crusts. The evaluation model was developed by modifying the model for the manganese nodules. In addition to considering the geological and geophysical differences between the manganese nodules and the cobalt-rich manganese crusts, an ore dressing subsystem was installed in the model. The mining subsystem is composed of a self-propelled collector--a pipeline with submersible hydraulic pumps for crust lifting. The smelting and chlorine leach method was selected for metallurgical processing. The production scales were established at 2,500t/y of cobalt metal. The production of three metals--cobalt, nickel, and copper--was considered in terms of metallurgical processing. The economic feasibility analyses demonstrated that the payback period was 11.4 years, the NPV was 36M$, and the IRR was 9.6% with the economic factors in the case of a cobalt price of US$ 25/lb. It was also demonstrated in this study that the payback period was 8.6 years, the NPV was 154M$, and the IRR was 14.0% in the case of a cobalt price of US$ 30/lb. This indicates that the approach under consideration appears to offer greater potential given the predicted metal prices.

• Geomechanics and Engineering
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• 제3권3호
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• pp.189-206
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• 2011

Amplification based on empirical relations is widely used for seismic microzonation of urban centers. Amplifications are used to represent the site effects of a particular soil column. Many empirical correlations are available to estimate the amplification of seismic waves. These correlations are based on the ratio of shear wave velocity of foundation/rock to soil velocity or 30 m equivalent shear wave velocity ($Vs^{30}$) and are developed considering deep soil data. The aim of this work is to examine the applicability of available amplification relations in the literature for shallow engineering bedrock sites by carrying out site response studies. Shear wave velocity of thirteen sites having shallow engineering bedrock have been selected for the study. In these locations, the depth of engineering bedrock (> 760 ${\pm}$ 60 m/s) is matched with the drilled bore hole. Shear wave velocity (SWV) has been measured using Multichannel Analysis of Surface Wave survey. These sites are classified according to the National Earthquake Hazards Reduction Program (NEHRP) classification system. Amplifications for an earthquake are arrived for these sites using empirical relations and measured SWV data. Site response analysis has been carried out in SHAKE using SWV and using synthetic and real earthquake data. Amplification from site response analysis and empirical relations are compared. Study shows that the amplification arrived using empirical relations does not match with the site response amplification. Site response amplification is much more than empirical values for same shear wave velocity.

• 지구물리
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• 제9권4호
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• pp.343-349
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• 2006

소양댐 상류의 미고결 퇴적물 분포를 파악하기 위하여, 길이 94 m의 5개 측선을 따라 2 m 간격으로 204 ms동안 탄성파 자료를 기록하였다. 기록된 자료를 초동주시 토모그래피 역산법과 지연시간법으로 처리하여 조사지의 퇴적물 분포를 종합적으로 구명하였다. 기반암은 평균 14 m 깊이로 비교적 평탄하게 분포하며, 산사면이 있는 남동쪽으로 상승한 형태를 보인다. 이 기반암을 댐 건설 이전에 형성된 기존 퇴적물이 덮고 있으며, 주로 호수 생성 이전에 형성된 토양이나 사질 퇴적물로 구성되어 있다. 최상부층인 최신 퇴적물은 호수 생성 이후 유입된 부유 퇴적물 기원의 이질 퇴적층으로, 하류지역보다 두꺼운 평균 1.6 m 두께로 쌓여 있다.