• Nuclear Engineering and Technology
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• v.23 no.4
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• pp.444-455
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• 1991

An accurate and fast running NEDAR model for calculating radial power profile throughout fuel life in both solid and annular pellets for existing and advanced CANDU-PHWR-fuel was developed in this work. This model contains resultant flux depression equations and neutron depression data tables which have been developed for CANDU-PHWR fuel of pellet with the diameter 8.0 to 19.5 mm and enrichment 0.71-6.0 wt % U-235, over a bumup range of 0 to 840 MWh /kgU (35000 MWD/T). In order to obtain the neutron flux distribution in the fuel pellet, the CE-HAMMER physics code was run for a neutron flux spectrum appropriate to a CANDU-PHWR to give predictions of radial power profile for several ranges of fuel design parameters. The results, which were calculated by the CE-HAMMER physics code, were fitted to an equation which is solved in terms of Bessel and exponential functions in order to obtain the parameters, $textsc{k}$, $\beta$ and λ in the resultant equation. The present NEDAR model produce a radial profile which, when normalized to unity at the pellet surface, is slightly higher than the profile of the original ELESIM data table. The predictions of the fission gas release by KAFEPA-NEDAR are in slightly better agreement with the experiments than those of ELESIM. The NEDAR model described in this study has been shown to provide an effective, reliable, and accurate method for determining radial power profiles in CANDU-PHWR fuel rods without incurring a significant increase in computing time.

• The Proceedings of the Korean Institute of Illuminating and Electrical Installation Engineers
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• v.3 no.2
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• pp.51-55
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• 1989

전원주파수 5-13[KHz]로 구동되는 형광램프(38mm 40W) 양광주 내의 수은의 여기원자 밀도를 시간과 반경방향에 대하여 계산하였다. 계산과정에서 수은의 에너지 준위는 기저 준위, 63P0, 63P1, 63P2와 이온화 준위가 고려되었으며, 전자의 에너지 분포함수는 2 Electron Group Model이 사용되었다. 계산결과는 일반적으로 사용하는 반경방향의 여기원자 밀도가 포물선 혹은 0차 Bessel 함수 형태라는 가정과 크게 다른 것으로 나타났다.

• The Proceedings of the Korean Institute of Illuminating and Electrical Installation Engineers
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• v.7 no.2
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• pp.31-35
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• 1993

The radial density distributions of the positive column of strongly modulated low -pressure gas discharges in mercury - rare gas mixtures at 10 tom pressure have been studied theoretically. The current was modulated inusoidally with a modulation depth of 50%. Calculations have shown that the radial profile of the excited atoms is ditferent form 0th Bessel function $J_0$(2.4r/R) and the invertion of the radial distribution of the excited atom can occur at some frequency. The hybrid method of FDM and 2nd order Runge-Kutta meth od is used for solving differenzial equations.

• Journal of Korean Ophthalmic Optics Society
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• v.16 no.4
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• pp.439-444
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• 2011

Purpose: To represent the shape of toric corea in the elliptical function for the determination of curvature distribution and lacrimal thickness between cornea and contact lens when the lens is fitted. Methods: Topography measurements of corneal curvature and curvature equation derived from the assumed elliptical function were evaluated using the Excel program which included the necessary equation derived. Results: Mathematical expressions for the cornea whose ribbon shaped-topography image, in which the center does not coincide with the corneal apex, can be determined. Conclusions: For the application where the higher accuracy on the cornea is not required, such as higher order aberration, the cornea cal be expressed in the simple elliptical function.

• Journal of the Korean Institute of Illuminating and Electrical Installation Engineers
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• v.13 no.4
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• pp.82-86
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• 1999

Electron Energy Distribution Function(EEDF) were treasured In Radio-Frequency Inductively Coupled Plasma(RFlCP) using a probe rrethocl Measurerrents were conducted in argon discharge for pressure from 10[mTorr] to 4O[mTorr] and input rf power from 100[W] to 600[W] and flow rate from 3[sccm] to 12[sccm]. Spatial distribution of electron energy distribution function were measured for discharge with same aspoct ratio (R/L=2). Electron energy distribution function strongly depended on both pressure and power. Electron energy distribution function increased with increasing flow rate. Radial distribution of the electron energy distribution function were peaked in the plasma center. Normal distribution of the electron energy distribution function were peaked in the center between quartz plate and substrate. From the results, we can find out the generation mechanism of Radio Frequency Inductively Coupled Plasma. And these results contribute the application of a simple Inductively Coupled Plasma(ICP).a(ICP).

• Proceedings of the Korea Electromagnetic Engineering Society Conference
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• 2001.11a
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• pp.12-15
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• 2001

본 논문에서는 무한 도체판에 존재하는 폭이 좁은 슬롯에 단락도체를 설치하였을 때 슬롯을 통하여 침투하는 침투전자파의 크기를 검토하고 있다. 이론해석으로서는 슬롯 개구면의 전계분포에 관한 적분방정식을 유도하고, 개구면 전계분포를 등가 반경의 개념을 적용한 선자류로 가정하여 구분정현함수를 사용한 Galerkin의 모멘트법으로 침투전자파의 크기를 계산하였다. 슬롯에 평면파가 입사할 때 슬롯 개구에 설치된 단락도체에 의해 개구면 전계분포가 제어되고 침투전자파의 크기가 감소된다는 것을 확인하고 있다.

• Bulletin of the Society of Naval Architects of Korea
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• v.27 no.2
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• pp.13-20
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• 1990

The interaction of the flows induced by stator blades with a ship-like wake is discussed to obtain the flow components of each with and without radial shear. The flow induced by stator blades is modeled by lifting line theory and the shear is taken to be provided by the radial gradient of the peripheral mean axial flow approximated by a logarithmic function of radius for a class of vessels. And the theory is based on the linearized Euler equations in the absence of viscosity. The results show that shear effects are relatively large at inner radii and the distribution of blade pitch angles is most effective in reducing non-uniformity.

• The Bulletin of The Korean Astronomical Society
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• v.37 no.1
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• pp.56.1-56.1
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• 2012

구경 3.6m CFHT 관측으로 얻은 산개성단 NGC 1245와 NGC 2506의 측광결과를 이용하여 두 성단의 역학적 진화와 헤일로 구조를 연구하였다. 이를 위하여 우리는 별들의 색-등급 도상의 위치와 천구 상에서의 위치를 동시에 고려하여, 각 별들에 대한 측광학적 구성원 확률을 정의하는 방법을 개발하였다. 이 방법을 사용하여 얻어진 구성원 확률을 이용하여 성단의 반경에 따른 구성원 별들의 광도함수와 반경에 따른 별들의 유효개수밀도 분포를 구하였다. 이들로부터 우리는 두 성단에서 질량분리현상을 확인하였으며, 성단에서 증발한 별들에 의해 형성된 헤일로의 존재를 알 수 있었다. 또한, 각 성단들의 공간상에 투영된 유효개수밀도 분포를 분석하여, 두 성단 모두 형태가 찌그러져 있으며 그 방향은 은하면과 관련이 적음을 보였다. 본 발표에서는 새로 개발한 구성원 확률을 정의하는 방법 및 두 성단의 역학적 진화와 헤일로 구조에 대한 내용을 소개하고자 한다.

• Journal of Korean Society of Forest Science
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• v.86 no.1
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• pp.17-24
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• 1997

As the first step to estimate the potential natural vegetation distribution of the globe, the best spherical interpolation method was developed to the temperature and precipitation which have close relation to the distribution pattern of world natural vegetation. For developing the interpolation method, a named Light Climatic Dataset composed of 1,060 stations around the globe was randomly divided into halves of feeding side and target side. The discrepancy between the observed and estimated values at the target stations was compared with combinations of parameters and methods. The estimated values were calculated to each combination which is all-out, constant radius and constant station methods in the selection of the feeding stations, n square reciprocal and negative exponential functions in weighting function of distance between feeding stations and each target, and oval weighting in direction of the feeding stations from each target. As a result, it turned out that the spherical interpolation with negative exponential weighting function fed from the constant radius stations ovally weighed yields the best estimates both for temperature and for precipitation. The parameters for temperature are $30^{\circ}$ in constant radius, 0.78 in negative exponential function and 0.4 in oval weighting, and for precipitation are $30^{\circ}$, 0.53 and 0.4, respectively.

• Journal of Intelligence and Information Systems
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• v.6 no.1
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• pp.65-72
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• 2000

In this paper we propose the new binary image matching algorithm called the Fuzzy logic induced Hausdorff Distance(FHD) for finding the maximally matched image with the query image. The membership histogram is obtained by normalizing the cardinality of the subset with the corresponding radius after obtaining the distribution of the minimum distance computed by the Hausdroff distance between two binary images. in the proposed algorithm, The fuzzy influence method Center of Gravity(COG) is applied to calculate the best matching candidate in the membership function described above. The proposed algorithm shows the excellent results for the face image recognition when the noise is added to the query image as well as for the character recognition.