• Proceedings of the KIEE Conference
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• 2005.07c
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• pp.2082-2084
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• 2005

I-V 특성 곡선의 2차 미분을 통해서 얻어지는 전자 에너지 분포 함수를 정확하게 구하기 위해서는 스무딩 과정이 반드시 필요하다. 대표적인 스무딩 방법으로 가우시안 확률 밀도 함수를 instrument함수로 이용하는 가우시안 스무딩이 있다. 본 연구에서는 시스템에 따라서 instrument함수가 다르다는 점에 착안하여, 여러 가지 다른 종류의 확률 밀도 함수를 instrument함수로 사용 스무딩에 적용하여 확률 밀도 함수에 따른 노이즈 제거 및 전자 에너지 분포 함수의 정확도를 비교하였고. 동시에 대표적인 범용 스무딩 방법인 사비츠키-골래이 스무딩, Polynomial fitting과도 그 결과를 비교 분석하였다.

• Proceedings of the Korean Vacuum Society Conference
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• 2016.02a
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• pp.214.1-214.1
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• 2016

최근 대기압 플라즈마의 활용분야는 기판의 표면처리, 바이오 분야 등에 널리 활용되고 있지만, 현재까지 정립된 대기압 플라즈마 분석법은 광학적, 전기적 방법으로 이를 통해 대기압 플라즈마를 분석하는데 어려움을 겪고 있다. 가장 널리 사용되는 OES(Optical Emission Spectroscopy) 측정법의 경우에는 플라즈마로부터 방출되는 광을 측정하여, 방출 강도로부터 플라즈마 밀도를 얻는데 어려운 점이 있다. 전기적 진단법 중 하나인 랑뮤어 탐침은 주로 진공장비에서만 사용가능하며, 대기압플라즈마에서 직접 접촉하여 플라즈마에 영향을 주어, 플라즈마 밀도를 정확히 측정하기 어렵다. 본 연구에서는 대기압 플라즈마의 캐페시턴스을 측정하여 플라즈마의 밀도를 측정하였다. DC power supply에서 발생된 DC전원을 인버터를 통해서 AC전원으로 변환한 뒤, Ar가스를 석영관에 주입하여 대기압 플라즈마 젯를 발생시켰다. 발생된 대기압 플라즈마를 석영관 외부 전극 사이에 캐패시턴스로 플라즈마 밀도를 측정하였다. Ar 가스 유량에 따라 플라즈마 밀도를 변화를 살펴보았다.

• Journal of Astronomy and Space Sciences
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• v.19 no.2
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• pp.123-132
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• 2002

The electron density and temperature in the topside ionosphere are observed by the ionosphere Measurement Sensor (IMS) onboard the KOMPSAT-1, which has the sun-synchronous orbit of the altitude of 685 km and the orbital inclination of $98^{\circ}$ with a descending node at 22:50LT. Observations have been analyzed to determine the seasonal variations of the electron density and temperature in the low-latitude region. Only the night-time (22:50LT) behavior on magnetically quiet days (Kp < 4) has been examined. Observations show a strong longitudinal and seasonal variation. Generally, in the dip equator the density increases and the temperature decreases. In equinox the latitudinal distributions of the electron density and temperature are quite symmetric about the dip equator. However, the local maximum of the density and the local minimum of the temperature shift toward the Northern hemisphere in summer solstice but the Southern hemisphere in winter solstice. Such variations are due to the influences of field-aligned plasma transport induced by F region neutral wind. Compared with the IRI95 model, the observed electron density and temperature show significant differences from those predicted by the IRI95 model.

• Journal of Korean Society of Transportation
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• v.24 no.5 s.91
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• pp.135-142
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• 2006

The flow-density relations represent equilibrium relations between flow and density in the stationary state. Using individual vehicle data this paper proposed a method to 131ter traffic data in the stationary state and showed flow-density relations produced by the traffic data in the stationary state. The Proposed method is based on the idea that free flow and congested flow show totally different traffic behaviors and time series of the traffic data observed at detection stations. The traffic data collected from the stationary state in the free flow using this filtering method consist in the left branch of the flow-density relation and the traffic data collected from the stationary state in the congested flow consist in the right branch of the flow-density relation. The traffic data in the stationary state skew reproducible flow-density relation in the almost whole range of the traffic flow.

• Journal of Korean Society of Coastal and Ocean Engineers
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• v.5 no.4
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• pp.302-306
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• 1993

Assuming Gaussian distribution of the density difference between a turbulent jet river plume and its ambient saline water, a hydrodynamic solution for the lateral spreading of a river plume is developed. Two advantages can be expected from the assumption we made. Firstly, we need not consider mixing processes in the plume in dealing with this Problem. Secondly, by Putting pressure gradients which can be obtained from the density distribution, into the equation of motion, we can solve them easily. We compared the analytic solution with the fold data of the Nakdong river plume and found reasonably good correspondence.

• Journal of the Korean Vacuum Society
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• v.17 no.3
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• pp.226-233
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• 2008

The nucleation and evolution process of Ge nano-islands on Si(001) surfaces grown by chemical vapor deposition have been explored using atomic force microscopy (AFM). The Ge nano-islands are grown by exposing the substrates to a mixture of gasses GeH4 and H2 at pressure of 0.1-0.5Torr and temperatures of $600-650^{\circ}C$. The effect of growth conditions such as temperature, Ge thickness, annealing time on the shape, size, number density, and surface distribution was investigated. For Ge deposition greater than ${\sim}5$ monolayer (ML) with a growth rate of ${\sim}0.1ML/sec$ at $600^{\circ}C$, we observed island nucleation on the surface indicating the transition from strained layer to island structure. Further deposition of Ge led to shape transition from initial pyramid and hut to dome and superdome structure. The lateral average size of the islands increased from ${\sim}20nm$ to ${\sim}310nm$ while the number density decreased from $4{\times}10^{18}$ to $5{\times}10^8cm^{-2}$ during the shape transition process. In contrast, for the samples grown at a relatively higher temperature of $650^{\circ}C$ the morphology of the islands showed that the dome shape is dominant over the pyramid shape. The further deposition of Ge led to transition from the dome to the superdome shape. The evolution of shape, size, and surface distribution is related to energy minimization of the islands and surface diffusion of Ge adatoms. In particular, we found that the initially nucleated islands did not grow through long-range interaction between whole islands on the surface but via local interaction between the neighbor islands by investigation of the inter-islands distance.

• Proceedings of the Korean Vacuum Society Conference
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• 2013.08a
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• pp.227-227
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• 2013

본 연구에서는 Si(111) 기판에 성장온도 및 InN 증착양 변화에 따른 InN 양자점(Quantum Dot) 핵성생(Nucleation) 특성에 대해 논의한다. InN 양자점은 Nitrogen-Plasma 소스를 장착한 분자선증착기(MBE)를 이용하여 $0.103{\AA}/s$의 성장속도로 성장하였다. 성장온도를 $700^{\circ}C$에서 $300^{\circ}C$로 변환하면서 형성한 시료에서 lnN 양자점의 공간밀도는 $9.4{\times}10^7/cm^2$부터 $1.1{\times}10^{11}/cm^2$를 나타냈다. 가장 높은 공간밀도인 $1.1{\times}10^{11}/cm^2$는 기존에 보고된 값 ($7.7{\times}10^{10}/cm^2$)보다 상대적으로 높은 값을 갖는다 [1,2]. InN 증착양을 93, 186, 및 $372{\AA}/s$으로 각각 변화시켜 형성하여 양자점의 초기 성장거동을 분석하였다. InN 증착양이 증가함에 따라 양자점의 공간밀도는 $4.4{\times}10^{10}/cm^2$에 $6.4{\times}10^{10}/cm^2$까지 증가하였다. 일반적으로 InP 및 GaAs 기판을 기반으로 한 In(Ga)As 양자점은 증착양이 증가함에 따라 밀도는 감소하고 크기는 증가하는 경향을 보이며, 이는 같은 상 (Phase)을 갖는 물질들끼리 결합하려는 경향이 있기 때문이다. 본 실험에서는 기존 결과와 다른 경향을 보이고 있는데, 이는 Si(111) 기판과 InN 사이의 격자부정합이 상대적으로 크기 때문에 InN 양자구조가 커지는 대신 추가로 새로운 핵생성 메커니즘에 의한 것으로 설명할 수 있다. 이러한 InN 증착양에 따른 InN 양자점 성장거동을 표면에너지를 포함한 이론적인 모델을 통해 논의하고자 한다.

• Journal of Korean Society of Forest Science
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• v.84 no.4
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• pp.409-414
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• 1995

This study was carried out for the analysis and comparison about the noise diminution effects by the height, width and density of Euonymus japonica wall, the distance of sound source, the distance of sound receiver, the height of sound source, and the height of sound receiver. The results obtained were summarized as follows; 1. After the establishment of tree wall, the volume of noise diminution measured 6.8dB and the effects of noise diminution measured heigher than before by 10.6% and t-value was significant at the 1% level 2. In simple correlation between the effects of noise diminution and variables, the density of tree wall was found as the most significant factor, and the last were found in the order of the distance of sound receiver, the width of tree wall, and the distance of sound source. 3. In partial correlation coefficients the effects of noise diminution and variables, the density of tree wall (r=-0.959) was found as the most significant factor, and the last were found in order of the distance of sound receiver (r=-0.906) and the width of tree wall (r=-0.753). 4. The estimated equation to measure the effects of noise diminution according to variables (the height of tree wall, the width of tree wall, the density of tree wall, the distance of sound source, the distance of sound receiver, the height of sound source, and the height of sound receiver) was $Y=69.520-1.672X_1-1.656X_2-0.066X_3-0.248X_4-3.134X_5-0.222X_6-0.343X_7$, and the coefficient of determination of this estimated equation was highly found as 0.950. 5. In semi-partial correlation coefficient the effects of noise diminution were found in the order of the density of tree wall, the distance of sound receiver, the width of tree wall, and the height of tree wall from the highest to the lowest. Therefore, it was considered that the density of tree wall, the distance of sound receiver, the width of tree wall and the distance of sound source should be controlled effectively to increase the effects of noise diminution by Euonymus japonica wall.

• Journal of the Korean earth science society
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• v.26 no.7
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• pp.691-697
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• 2005

Recently, the development of accurate gravity-meter and GPS make it possible to obtain high resolution gravity data. Though gravity data interpretation like modeling and inversion has significantly improved, gravity data processing itself has improved very little. Conventional gravity data processing removes gravity effects due to mass and height difference between base and measurement level. But, it would be a biased density model when some or whole part of anomalous bodies exist above the base level. We attempted to make a multiquadric surface of the survey area from topography with DEM (Digital Elevation Map) data. Then we constituted rectangular blocks which reflect real topography of the survey area by the multiquadric surface. Thus, we were able to carry out 3-D inversions which include information of topography. We named this technique, 3-D Gravity Terrain Inversion (3DGTI). The model test showed that the inversion model from 3DGTI made better results than conventional methods. Furthermore, the 3-dimensional model from the 3DGTI method could maintain topography and as a result, it showed more realistic geologic model. This method was also applied on real field data in Masan-Changwon area. Granitic intrusion is an important geologic characteristic in this area. This method showed more critical geological boundaries than other conventional methods. Therefore, we concluded that in the case of various rocks and rugged terrain, this new method will make better model than convention ones.

• Proceedings of the Korean Vacuum Society Conference
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• 2013.02a
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• pp.529-529
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• 2013

플라즈마를 진단하는 데에는 장비적으로나 현실적으로 많은 제약이 따른다. 따라서 측정 할 수 있는 parameter가 적다. 그리고 진단 장비의 성능에 따라서 측정된 data의 신뢰도가 결정된다. 그래서 플라즈마에 레이저를 쏘아서 생성되는 솔리톤의 RADIATION을 이용하여 플라즈마의 특성을 파악하려고 한다. 본 시뮬레이션은 Particle-In-Cell (PIC) 시뮬레이션을 이용하여 Underdense 플라즈마에 Terahertz 레이저를 쏘았을 경우 발생되는 솔리톤의 특성을 파악하였다. 2D 시뮬레이션으로 수행하였으며 플라즈마는 Underdense 플라즈마를 이용하였다. 레이저 Focusing 점의 위치와 솔리톤의 주파수, 플라즈마의 밀도 gradient 에 따른 솔리톤의 이동 및 특징, 플라즈마 밀도에 따른 솔리톤의 특징을 살펴보았다.