• Proceedings of the Korean Institute of Surface Engineering Conference
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• 2015.05a
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• pp.186-186
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• 2015

레이저 홀로그램에서 추출한 입자 데이터와 Langmuir probe로 측정한 이온 플럭스간의 개선된 상관관계를 보고한다. 레이저 홀로그램 센서 시스템을 이용하여 척 온도 변화에 따른 플라즈마 공간에서의 입자에너지 분포를 이미징하였다. 진공에너지분포를 뺀 에너지분포에 나타나는 두 종류의 분포에 관여하는 전체 입자수 분포는 이온플럭스 데이터와 전체 온도 범위에서 매우 유사한 경향성을 보였다.

• Proceedings of the Membrane Society of Korea Conference
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• 1997.04b
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• pp.48-49
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• 1997

막분리에 있어 막오염 현상은 공정의 경제성을 좌우하는 중요한 요소이다. 이에따라 막오염에 따른 플럭스 변화를 예측하기 위한 다양한 방법을 시도하고 있다. 그러나 대부분의 동력학적 해석식들은 여과초기에만 적용되는 단점이 있었다. 최근에는 콜로이드 입자에 의한 막오염 과정을 그대로 모사하여 여과개시 후 상당한 시간 후의 플럭스를 예측하려는 시도를 하고 있다. 그러나 지금까지 연구된 모델들은 2차원입자를 사용하거나 혹은 단일입자분포를 갖는 3차원입자를 사용한 것들이었다. 2차원 모사인 경우 세공막힘현상을 설명할 수 없으며 3차원 단일분포 입자시스템은 현실과는 거리가 먼 단점이 있었다. 이에따라 본 연구에서는 다중분포(multi-disperse)를 갖는 입자의 정밀여과 (microfiltration)를 모사하여 시간에 따른 플럭스의 변화를 예측해 보고자 하였다.

• The Bulletin of The Korean Astronomical Society
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• v.37 no.2
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• pp.124.2-124.2
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• 2012

위성체의 전위는 위성 주변의 우주 환경에 크게 영향을 받는다. 본 연구에서는 과학기술위성 1호(STSAT-1)에 탑재된 LP(Langmuir Probe)와 ESA(Electro-Static Analyzer) 관측 자료를 이용하여 위성체의 전위에 위성 주변 고에너지 입자들이 미치는 영향을 분석하였다. 일반적으로 위성체가 대전되어 위성체의 부동전위가 감소할 때 위성 주변의 플라즈마 밀도는 감소하고 온도는 증가한다. 또한 DMSP 위성 등을 비롯한 이전 관측에서는 고에너지 입자의 플럭스가 증가하는 지역을 위성이 통과할 때 위성체의 전위가 감소하였다. 본 연구에서는 위성이 수 ~ 수 십 keV 정도의 고에너지 입자 플럭스가 증가한 후 감소하는 지역을 통과할 때에도 위성체의 전위가 감소하는 현상을 관측하였다. 고에너지 입자의 플럭스가 감소하는 지역에서 일어나는 위성의 대전현상을 통계적으로 분석해 보고 이러한 결과를 토대로 위성체 전위 변화에 우주환경 변화가 어떤 영향을 주는지 연구하였다.

• The Bulletin of The Korean Astronomical Society
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• v.37 no.2
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• pp.129.1-129.1
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• 2012

서포트 벡터 머신(Support Vector Machine, SVM)과 인공신경망 모형(Neural Network, NN)을 사용하여 태양 양성자 현상(Solar proton event, SPE)의 플럭스 세기를 예측해 보았다. 이번 연구에서는 1976년부터 2011년까지 10MeV이상의 에너지를 가진 입자가 10개 cm-1 sec-1 ster -1 이상 입사할 경우를 태양 양성자 현상으로 정의한 NOAA의 태양 고에너지 입자 리스트와 GOE위성의 X-ray 플레어 데이터를 사용하였다. 여기에서 C, M, X 등급의 플레어와 관련있는 178개 이벤트를 모델의 훈련을 위한 데이터(training data) 89개와 예측을 위한 데이터(prediction data) 89개로 구분하였다. 플러스 세기의 예측을 위하여, 우리는 로그 플레어 세기, 플레어 발생위치, Rise time(플레어 시작시간부터 최대값까지의 시간)을 모델 입력인자로 사용하였다. 그 결과 예측된 로그 플럭스 세기와 관측된 로그 플럭스 세기 사이의 상관계수는 SVM과 NN에서 각각 0.32와 0.39의 값을 얻었다. 또한 두 값 사이의 평균 제곱근 오차(Root mean square error)는 SVM에서 1.17, NN에서는 0.82로 나왔다. 예측된 플럭스 세기와 관측된 플럭스 세기의 차이를 계산해 본 결과, 오차 범위가 1이하인 경우가 SVM에서는 약 68%이고 NN에서는 약 80%의 분포를 보였다. 이러한 결과로부터 우리는 NN모델이 SVM모델보다 플럭스 세기를 잘 예측하는 것을 알 수 있었다.

• Membrane Journal
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• v.7 no.3
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• pp.150-156
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• 1997

The particle back transport velocity from the membrane surface were evaluated to determine the critical flux. Four kinds of back transport mechanisms were considered, i.e. back diffusion, shear induced migration, lateral migration, and interaction enhanced migration. The interaction enhanced migration caused by electrostatic repulsion between particles and membrane surface was found to be the most important mechanism of particle back transport for the charged particles of 0.1 ~10${\mu}{\textrm}{m}$ diameter with 20 to 40 mV of zeta potential. Hematite particles with different sizes were synthesized with ferric chloride (FeCl$_3$) and hydrochloric acid (HCl) at high temperature, and subsequently experimental critical fluxes for each sized particle were obtained. The experimental results were well coincident with the calculated critical fluxes based on back transport mechanisms.

• Journal of Astronomy and Space Sciences
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• v.23 no.3
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• pp.217-226
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• 2006

We report three sawtooth oscillation events observed at geosynchronous orbit where we find quasi-periodic (every 2-3 hours) sudden flux increases followed by slow flux decreases at the energy levels of ${\sim}50-400keV$. For these three sawtooth events, we have examined variations of the outer boundary of the outer radiation belt. In order to determine L values of the outer boundary, we have used data of relativistic electron flux observed by the SAMPEX satellite. We find that the outer boundary of the outer radiation belt oscillates periodically being consistent with sawtooth oscillation phases. Specifically, the outer boundary of the outer radiation belt expands (namely, the boundary L value increases) following the sawtooth particle flux enhancement of each tooth, and then contracts (namely, the boundary L value decreases) while the sawtooth flux decreases gradually until the next flux enhancement. On the other hand, it is repeatedly seen that the asymmetry of the magnetic field intensity between dayside and nightside decreases (increases) due to the dipolarization (the stretching) on the nightside as the sawtooth flux increases (decreases). This implies that the periodic magnetic field variations during the sawtooth oscillations are likely responsible for the expansion-contraction oscillations of the outer boundary of the outer radiation belt.

• Journal of the Institute of Electronics and Information Engineers
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• v.52 no.3
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• pp.105-115
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• 2015

In semiconductor etching simulation, The source modeling for generating plasma species is required. In this paper, we modeled the source of plasma etching process with probability distribution and the feature profile with simple geometry objects, then got the flux on the feature profile. The distance between the source and the cell on the modeling parameters of the source, there are a number of particles to be emitted from a source, there is a number (area of the cell) of the cell on the profile with additional parameters to give the calculation of flux. The flux error ratio on both gaussian(Incident Flux) and cosine probability distribution(Incident Neutral Flux) is much decreased as the number of ray is increased but the processing time is more increased than that. The increase of the number of cell and distance makes increase the flux error ratio and the processing time moderately. In view of the processing time through the experimental results in this paper, it is possible to analogize the calculation of appropriate fluxes.

• Membrane Journal
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• v.8 no.2
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• pp.94-101
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• 1998

The oil separation is effectively performed from the oil containing alkaline cleaner solution by using a backflushed ultrafiltration system, where hollow fibers commercially made by polyacrylonitrile copolymer are bundled. Backflushing to reduce membrane fouling during crossflow ultrafiltration is investigated. Experimental observations allow us to understand the behavior of permeate flux according to the relative operating conditions, and determine the optimum condition of normal operation and backflushing. The maximum improvement of net permeate flux owing to backflushing was found to be about 23 % with the condition of 10 min/40 sec for the cycle of normal/backflushing operations. Note that, however, the maintenance of stable permeate flux is lost as the duration of normal operation is increased. The permeate flux depends on both the backflushing pressure and the feed flow rate. It is obvious that there is a critical velocity of feed flow, in which permeate flux is practically independent of backflushing pressure. Above this critical value, the permeate flux is proportional to an appropriate power of the backflushing pressure, $\Delta P_{back}^n$, where exponent n is enhanced with increasing feed velocity.

• Korean Chemical Engineering Research
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• v.51 no.1
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• pp.98-105
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• 2013

The NaA zeolite particles were dispersed in a poly(vinyl alcohol) (PVA) matrix to prepare a composite membrane. The nano sized zeolite particles of NaA were synthesized in the laboratory and the mean size was approximately 60 nm. Pervaporation characteristics such as a permeation flux and a separation factor were investigated using the membrane as a function of the feed concentration from 0.01 to 0.05 mole fraction and the weight % of NaA particles between 0 wt% and 5 wt% in the membrane. Also, the micro sized particles of $5{\mu}m$ were dispersed in the membrane for a comparison purpose. When the ethanol concentration in the feed solution was 0.01 mole fraction, the flux of water significantly increased from $600g/m^2/hr$ to $2000g/m^2/hr$ as the content of the nano NaA particles in the membrane increased from 0 wt% to 5 wt%, while the NaA particles improved the separation factor from 1.5 to 7.9. When the flux of water through the membrane containing nano sized particles was roughly 15% increased compared to the micro sized particles, whereas the separation factor of water was found to be approximately 5% increased. It can be said that the role of the nano sized NaA particles is quite important since both the flux and the separation factor are strongly affected.

• The Sea:JOURNAL OF THE KOREAN SOCIETY OF OCEANOGRAPHY
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• v.13 no.3
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• pp.200-209
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• 2008

Particle fluxes were measured with a time-series sediment trap from July 2003 to June 2005 at the St. KOMO(KOMO; Korea Deep-Sea Environmental Study Long-Term Monitoring Station, $10^{\circ}30'N,\;131^{\circ}20'W$) in the northeastern Pacific. Total mass fluxes at a depth of 4,960 m showed distinct seasonal variations with high values in the winter(December-February) and spring(March-May) and low values in the summer(June-August) and fall(September-November). Biogenic origin fluxes also displayed distinct seasonal variations similar to total mass fluxes. Particularly, calcium carbonate fluxes in winter and spring were more than two times greater than those in summer and fall. The prominent seasonal variations of total mass and biogenic fluxes were closely related with the seasonal changes of primary production in the surface waters; in winter and spring, primary production increased due to the enhanced supply of nutrients below the surface mixed layer by strong wind and less stratification, whereas it decreased as a result of the less supply of nutrient by reduced wind speed and strong stratification in summer and fall. The seasonal variations of total mass and biogenic fluxes in this study were higher than the differences of total mass and biogenic fluxes caused by the environmental changes such as El $Ni\tilde{n}o$ and La $Ni\tilde{n}a$ events in the previous studies. In order to understand the effects of El $Ni\tilde{n}o$ and La $Ni\tilde{n}a$ on the particle flux, therefore, the seasonal variation of particle flux in the northeastern equatorial Pacific needs to be well defined.