• 한국학교보건학회지
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• 제11권2호
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• pp.189-201
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• 1998

The objectives of this study are first to develop the index of school health promoting behaviors, two, to measure those, third, to analysis the relative importance of factors that effect on school health promoting behaviors. School health promotion indexes were composed of 60 components of six areas which modify the element of health promoting schools are developed by world health organization. The survey data were collected by questionnaires from June to September in 1998. The number of subjects was 294 school nurses. The SAS-PC program was used for the statistical analysis. The major results were as follows: 1. The six areas of school health promoting behaviors are: school health politics (20 components), the school physical environment (17 component), the school social environment (7 component), community relationships (6 component), personal health skills (7 component) and health services (3 component). 2. The mean of total school health promotion indexes was highest at elementary school as 3.46. The order of area was health services, the school physical environment, school health politics, the school social environment, personal health skills, community relationships. 3. The regression model used in this analysis presented significant relationships between school health promoting behaviors and independent variables. The important variable affecting the area of school physical environment was education level of school nurses. The important variable affecting the area of the school social environment and personal health services were the location of school, credential education program. Age or career also were significant variables affect the community relationships and health services. In summary, The health promoting behavior of elementary school was higher than other school. It is mean that have to perform active promoting behavior at middle school and high school. Health service level was highest among areas of school health promoting behaviors. It is mean also that school nurse teachers is interested in activity for other areas to improve of school health. Furthermore, it is necessary to develop the specific program for school health promoting behavior.

• 한국지반환경공학회 논문집
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• 제16권2호
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• pp.27-31
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• 2015

도심지 구간에 위치한 지반공학 관련 공사 현장에서는 충분한 안전율 확보와 더불어 사용성도 확보해야 한다. 이를 위해서는 공사 중 인접지반에 발생하는 변형을 제어해야 하므로 지반구조물과 관련된 기술 요구사항도 더욱 높아지고 있다. 사용성 확보를 위해서는 지반의 변형을 예측해야 하므로 지반의 강성을 분석해야 한다. 특히 강성의 비선형성과 이방성은 주요인자라 할 수 있다. 본 연구에서는 깊은 굴착 중 지반이 경험하는 응력경로에 따른 강성의 비선형성과 이방성에 대해 실내시험 결과와 전산 해석 결과를 비교하였다. 강성은 변형률이 작은 미소변형률 구간에서 비선형성이 두드러졌으며, 응력경로에도 큰 영향을 받는 것으로 나타났다. 실내시험 결과 압축은 작은 강성을 인장은 큰 강성을 나타내었으며, 깊은 굴착 시 지지벽체 뒤는 압축이 앞은 인장이 지배적인 응력경로를 나타내었다. 굴착 중 발생하는 지반의 변형을 정확히 예측하기 위해서는 지반이 경험하는 응력경로에 따라 변하는 강성의 변화 특성을 고려해야 한다.

• 대한기계학회논문집A
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• 제20권3호
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• pp.891-900
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• 1996

The vision sensor which is based on the optical triangulation theory with the laser as an auxiliary light source can detect not only the seam position but the shape of seam. In this study, a vision sensor using the scanning laser beam was investigated. To design the vision sensor which considers the reflectivity of the sensing object and satisfies the desired resolution and measuring range, the equation of the focused laser beam which has a Gaussian irradiance profile was firstly formulated, Secondly, the image formaing sequence, and thirdly the relation between the displacement in the measuring surface and the displacement in the camera plane was formulated. Therefore, the focused beam diameter in the measuring range could be determined and the influence of the relative location between the laser and camera plane could be estimated. The measuring range and the resolution of the vision sensor which was based on the Scheimpflug's condition could also be calculated. From the results mentioned above a vision sensor was developed, and an adequate calibration technique was proposed. The image processing algorithm which and recognize the center of joint and its shape informaitons was investigated. Using the developed vision sensor and image processing algorithm, the shape informations was investigated. Using the developed vision sensor and image processing algorithm, the shape informations of the vee-, butt- and lap joint were extracted.

• Spatial Information Research
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• 제23권6호
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• pp.89-98
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• 2015

본 연구에서는 공간정보를 활용하여 구현가능한 방범 관련 기능 및 서비스를 평가할 수 있는 기준을 도출하고, 도출된 기준별 상대적 중요도를 계산하여 최종적으로 공간정보 기반 지능형 방범서비스 어플리케이션의 적용 기능/서비스 대안에 대한 우선순위를 제시하였다. 또한 현재 정부 및 지자체 주도하에 운영 중인 10여개의 국민안심서비스의 연계방안과 세부 서비스 구현방안을 함께 제시함으로써 실질적인 사업화 및 실증화가 가능한 공간정보 기반 지능형 방범 앱서비스 모델을 제시하였다. 최종 평가기준은 1계층에 속하는 3가지와 2계층에 속하는 12가지의 평가기준에 따라 AHP 중요도 평가분석을 수행하였으며, 이를 토대로 긴급상황 시 대처방안, 보호자 실시간 위치파악 및 미아/치매환자전용 단말 사용, 사용자 참여 및 정보제공 등의 지능형 방범서비스 어플리케이션 구현방안을 모색하였다.

• 한국지리정보학회지
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• 제4권4호
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• pp.29-38
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• 2001

본 연구는 도시계획의 중요한 의사결정 중의 하나로서 토지이용계획을 위한 적지분석에 지리정보시스템의 접목을 시도한 것이다. 도 농 통합 이전의 구미시 지역을 대상지역으로 하여 관련 환경인자들과 가중치 등의 분석기준을 결정하고, GIS 데이터베이스를 구축하였다. 또한 위성영상처리를 통하여 추출한 토지이용/피복도와 NDVI 식생도를 데이터베이스에 포함시켰다. 중첩법을 이용하여 주거, 상업, 공업, 녹지지역의 토지용도별 적지를 등급별로 도출하였다. 연구지역의 4가지 기능공간에 대한 적지분석 결과는 기존 토지이용 및 도시기본계획상 토지이용구상도와 비교되었다. 더 나은 분석을 위해서는 실제적인 개발계획, 지가자료, 토양자료 등이 포함되어야 하며, 토지 이용별 수요추정 자료를 추가한다면 토지이용별 입지 배분 및 분포면적의 신뢰도를 더 높일 수 있을 것이다.

• 전자공학회논문지S
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• 제35S권11호
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• pp.12-18
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• 1998

비정지궤도 위성통신링크에서는 지표상의 단말기 또는 지구국 등에 대한 상대적인 위성의 이동으로 인하여 제공되는 위성 앙각이 시간에 따라 연속적으로 변한다. 따라서 비정지궤도 위성을 이용한 통신링크에서는 단말기가 일정 위치에 있을지라도 수신 신호가 받는 페이딩의 영향은 연속적으로 변한다. 본 논문에서는 비정지궤도 이동위성통신링크 사에서 발생하는 페이딩 특성을 전파 환경에 무관한 일반적인 통계적 함수로 모델을 정하고, 다양한 전파 환경에 대한 모델의 파라미터를 앙각의 함수로 설정하여, 상용 이동위성 통신 시스템의 페이딩 마진 데이터를 이용하여 파라미터 계수를 추출한다. 또한 구현된 모델을 이용하여 각 전파 환경에 따른 페이딩 특성을 분석한다. 분석된 결과는 이동위성통신 채널의 전송방식에 대한 성능 분석 및 페이딩으로 인한 신호 왜곡의 보상 알고리즘 개발에 활용가능할 것이다.

• 한국지능시스템학회논문지
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• 제26권2호
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• pp.160-167
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• 2016

본 논문은 천장 영상 정보를 이용한 이동 로봇 위치추정 방법을 제안한다. 지도상에 천장 영상의 랜드 마크의 위치는 미리 알고 있지만, 지도상의 랜드 마크와 감지된 랜드 마크 사이의 대응관계 정보는 주어지지 않는다. 단지, 로봇의 이동 시작 단계에서 랜드 마크들에 대한 상대적인 로봇의 위치가 주어진다. 로봇의 위치 및 천장 영상에서 감지된 특징점의 ID를 찾기 위해 파티클 필터 방법을 이용한다. 제안한 방법을 천장에 동일한 형태의 원형 랜드 마크를 가진 실내 환경에서 실험하여 성능을 검증하였다. 본 논문에서 제안한 위치추정 방법은 레이저 영역 센서에 의해 측정된 벽까지의 거리 또는 RF 나 초음파에 의해 측정된 비이컨까지의 거리 값에 큰 불확실성이 존재하는 물류 창고와 같은 환경에서 사용하기에 적합하다.

• Wind and Structures
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• 제26권3호
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• pp.147-161
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• 2018

For wind engineering applications downbursts are, presently, almost exclusively modeled, both experimentally and numerically, as transient impinging momentum jets (IJ), even though that model contains none of the physics of real events. As a result, there is no connection between the IJ-simulated downburst wind fields and the conditions of formation of the event. The cooling source (CS) model offers a significant improvement since it incorporates the negative buoyancy forcing and baroclinic vorticity generation that occurs in nature. The present work aims at using large-scale numerical simulation of downburst-producing thunderstorms to develop a simpler model that replicates some of the key physics whilst maintaining the relative simplicity of the IJ model. Using an example of such a simulated event it is found that the non-linear scaling of the velocity field, based on the peak potential temperature (and, hence, density) perturbation forcing immediately beneath the storm cloud, produces results for the radial location of the peak radial outflow wind speeds near the ground, the magnitude of that peak and the time at which the peak occurs that match well (typically within 5%) of those produced from a simple axi-symmetric constant-density dense source simulation. The evolution of the downdraft column within the simulated thunderstorm is significantly more complex than in any axi-symmetric model, with a sequence of downdraft winds that strengthen then weaken within a much longer period (>17 minutes) of consistently downwards winds over almost all heights up to at least 2,500 m.

• Restorative Dentistry and Endodontics
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• 제41권3호
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• pp.182-188
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• 2016

Objectives: The purpose of this study was to evaluate the proximity of the mandibular molar apex to the buccal bone surface in order to provide anatomic information for apical surgery. Materials and Methods: Cone-beam computed tomography (CBCT) images of 127 mandibular first molars and 153 mandibular second molars were analyzed from 160 patients' records. The distance was measured from the buccal bone surface to the root apex and the apical 3.0 mm on the cross-sectional view of CBCT. Results: The second molar apex and apical 3 mm were located significantly deeper relative to the buccal bone surface compared with the first molar (p < 0.01). For the mandibular second molars, the distance from the buccal bone surface to the root apex was significantly shorter in patients over 70 years of age (p < 0.05). Furthermore, this distance was significantly shorter when the first molar was missing compared to nonmissing cases (p < 0.05). For the mandibular first molars, the distance to the distal root apex of one distal-rooted tooth was significantly greater than the distance to the disto-buccal root apex (p < 0.01). In mandibular second molar, the distance to the apex of C-shaped roots was significantly greater than the distance to the mesial root apex of non-C-shaped roots (p < 0.01). Conclusions: For apical surgery in mandibular molars, the distance from the buccal bone surface to the apex and apical 3 mm is significantly affected by the location, patient age, an adjacent missing anterior tooth, and root configuration.

• 천문학회지
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• 제50권2호
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• pp.29-39
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• 2017

We investigate two abnormal CME-Storm pairs that occurred on 2014 September 10 - 12 and 2015 March 15 - 17, respectively. The first one was a moderate geomagnetic storm ($Dst_{min}{\sim}-75nT$) driven by the X1.6 high speed flare-associated CME ($1267km\;s^{-1}$) in AR 12158 (N14E02) near solar disk center. The other was a very intense geomagnetic storm ($Dst_{min}{\sim}-223nT$) caused by a CME with moderate speed ($719km\;s^{-1}$) and associated with a filament eruption accompanied by a weak flare (C9.1) in AR 12297 (S17W38). Both CMEs have large direction parameters facing the Earth and southward magnetic field orientation in their solar source region. In this study, we inspect the structure of Interplanetary Flux Ropes (IFRs) at the Earth estimated by using the torus fitting technique assuming self-similar expansion. As results, we find that the moderate storm on 2014 September 12 was caused by small-scale southward magnetic fields in the sheath region ahead of the IFR. The Earth traversed the portion of the IFR where only the northward fields are observed. Meanwhile, in case of the 2015 March 17 storm, our IFR analysis revealed that the Earth passed the very portion where only the southward magnetic fields are observed throughout the passage. The resultant southward magnetic field with long-duration is the main cause of the intense storm. We suggest that 3D magnetic field geometry of an IFR at the IFR-Earth encounter is important and the strength of a geomagnetic storm is strongly affected by the relative location of the Earth with respect to the IFR structure.