• 한국수자원학회논문집
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• 제47권2호
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• pp.119-133
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• 2014

본 연구에서는 Z-R 관계식의 매개변수를 안정적인 값으로 실시간 예측하고자 확장 칼만 필터기법을 적용하였다. 이를 위해 Z-R 관계식의 비선형을 고려하여 확장 칼만필터로 매개변수 결정모형을 구축하였다. 상태-공간모형은Adamowski and Muir (1989)의 연구를 기반으로 구축하였다. 상태-공간 모형의 상태변수는 Z-R 관계식의 두 매개변수로 설정하였다. 결과적으로 칼만이득과 상태변수가 발산하지 않는 안정적인 모형을 구축하였다. 주목할 점으로는 기존 방법으로 추정된 과대 혹은 과소한 매개변수가 필터링 되어 일부 제거되었다는 것이다. 부적절한 매개변수의 적용은 물리적으로 비현실적인 강우강도 추정 결과를 불러일으키는 원인이기 때문에 이러한 결과는 정량적 강수량 추정측면에서 효과가 크다고 할 수 있다. 또한 확장 칼만 필터로 예측한 매개변수로 레이더 강우를 추정한 결과, 편의보정계수가 1.0에 근사하게 나타나 편의보정과정 없이도 지상 강우강도와의 평균적인 차이는 근소한 것으로 나타났다. 또한 기존 방법으로 레이더 강우를 추정한 결과보다 전반적으로 정확도 높은 강우 추정이 가능한 것으로 나타났다.

• ETRI Journal
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• 제38권3호
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• pp.568-578
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• 2016

A wireless power transfer (WPT) system is usually classified as being of either a two-coil or four-coil type. It is known that two-coil WPT systems are suitable for short-range transmissions, whereas four-coil WPT systems are suitable for mid-range transmissions. However, this paper reveals that the two aforementioned types of WPT system are alike in terms of their performance and characteristics, differing only when it comes to their matching-network configurations. In this paper, we first find the optimum load and source conditions using Z-parameters. Then, we estimate the maximum power transfer efficiency under the optimum load and source conditions, and we describe how to configure the matching networks pertaining to both types of WPT system for the given optimum load and source conditions. The two types of WPT system show the same performance with respect to the coupling coefficient and load impedance. Further, they also demonstrate an identical performance in the two cases considered in this paper, that is, a strong-coupled case and a weak-coupled case.

• 천문학회보
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• 제43권2호
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• pp.41.1-41.1
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• 2018

We constrain cosmological parameters by combining three different power spectra measured from galaxy clustering, galaxy-galaxy lensing, and cosmic shear using the Deep Lens Survey (DLS). Two lens bins (centered at z~0.27 and 0.54) and two source bins (centered at z~0.64, and 1.1) containing more than one million galaxies are selected to measure the power spectra. We re-calibrate the initial photo-z estimation of the lens bins by matching with SHELS and PRIMUS and confirm its fidelity by measuring a cross-correlation between the bins. We also check the reliability of the lensing signals through the null tests, lens-source flipping and cross shear measurement. Residual systematic errors from photometric redshift and shear calibration uncertainties are marginalized over in the nested sampling during our parameter constraint process. For the flat LCDM model, we determine S_8=sigma_8(Omega_m/0.3)^0.5=0.832+-0.028, which is in great agreement with the Planck data. We also verify that the two independent constraints from the cosmic shear and the galaxy clustering+galaxy-galaxy lensing measurements are consistent with each other. To address baryonic feedback effects on small scales, we marginalize over a baryonic feedback parameter, which we are able to constrain with the DLS data alone and more tightly when combined with Planck data. The constrained value hints at the possibility that the AGN feedback in the current OWLS simulations might not be strong enough.

• Communications for Statistical Applications and Methods
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• 제10권3호
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• pp.749-764
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• 2003

In this paper we explain that normal theory likelihood-ratio tests(z, t, $x^2$. F) for mean(s) or variance(s) can be geometrically related to volume of difference of two joint pdf's. One is an estimated joint pdf under null parameter space $\omega$ and the other is an estimated joint pdf under full parameter space $\Omega$. For explanations, ‘distance between two distributions’ is defined. We study properties of it, and derive some results on the distance between two multivariate normal distributions.

• Progress in Superconductivity
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• 제2권1호
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• pp.6-10
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• 2000

New cuprates with the nominal composition $(Pb_{0.75}Sn_{0.25})Sr_2(Ca_{1-x}Lu_x)Cu_2O_z(x=0.4{\sim}1.0)$ have been synthesized. These materials exhibit superconducting properties for 0.4 $\leq$ x $\leq$ 0.7. It is also observed that the superconductivity of the as-prepared sample is enhanced by post-annealing at high temperature followed by quenching. X-ray diffraction analysis reveals that the c lattice parameter decreases as x increases whereas the a lattice parameter is nearly independent of the value of x for both the as-prepared and the post-treated samples. The thermoelectric power measurements indicate that the post-heat-treatments result in an increase in the hole carrier density which account for the observed increase of $T_c$. Bulk superconductivity with a $T_c$ value of 60 K is observed in this system.

• 한국복합재료학회:학술대회논문집
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• 한국복합재료학회 2002년도 춘계학술발표대회 논문집
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• pp.69-72
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• 2002

The high temperature deformation behavior of SiCp/2124Al composite and 2124Al alloy was investigated by hot compression test in a temperature ranged $400~475^{\circ}C$ over a strain rate ranged $10^{-3}~1s^{-1}$. The billets of 2124Al alloy and SiCp/2124Al composite were fabricated by vacuum hot pressing process. The stress-strain curve during high temperature deformation exhibited a peak stress, and then the flow stress decreased gradually into a steady state stress with increasing the strain. It was found that the flow-softening behavior was attributed to the dynamic recovery, local dynamic recrystallization and dynamic precipitation during the deformation. The precipitation phases were identified as S' and S by TEM diffraction pattern. Base on the TEM inspection, the relationship between the Z-H parameter and subgrain size was found based on the experiment data. The dependence of flow stress on temperature and strain rate could be formulated well by a hyperbolic-sinusoidal relationship using the Zener-Hollomon parameter.

• 대한전자공학회논문지SD
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• 제41권12호
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• pp.21-26
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• 2004

본 논문에서는 package된 BJT의 RF 등가회로 모델을 optimization과정 없이 직접 추출하는 방법을 개발하였다. 먼저, open 과 short package 구조를 사용하여 plastic package의 기생성분을 측정된 S-파라미터로부터 정확히 제거하였다. 이와 같이 package do-embedding된 S-파라미터로부터 package lead와 chip pad 사이의 bonding wire 인덕턴스와 chip pad 캐패시턴스를 직접 추출하는 간단한 방법을 구축하였다. 그 후에 내부 BJT소자의 소신호 모델변수들은 RF 등가회로로부터 유도된 Z나 Y-파라미터 방정식을 이용하여 결정하였다. 이 방법으로 모델화된 packaged BJT의 S-파라미터는 측정 데이터와 아주 잘 일치하였으며 이는 새로운 추출방법의 정확성을 증명한다.

• 대한수학회논문집
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• 제11권1호
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• pp.81-87
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• 1996

We will construct polynomials of degree 6 in z and $\bar{z}$ on $C^2$ which gives, via its coefficient $\beta$ as a parameter, a family of pseudoconvex domains $\Omega_\beta$ in $C^2$ with the origin being a boundary point, and show that the domains $\Omega_\beta$ has no peak functions of class $c^1$ at the origin and has no holomorphic support functions for $1 \leq \beta < \frac{9}{5}$.

• 천문학회보
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• 제40권1호
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• pp.47.2-47.2
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• 2015

At local, galaxy properties are well known to be clearly different in different environments. However, it is still an open question how this environment-dependent trend has been shaped. In this presentation, we will show the results of our investigation about the evolution of star-formation properties of galaxies over a wide redshift range, from z~2 to z~0.5, focusing its dependence on their stellar mass and environment. In the UKIDSS/UDS region, we estimated photometric redshifts and stellar population properties, such as stellar masses and star-formation rates, using the deep optical and near-infrared data available in this field. Then, we identified galaxy cluster candidates at z~0.5-2. Through the analysis and comparison of star-formation (SF) properties of galaxies in clusters and in field, we found interesting results regarding the evolution of SF properties of galaxies: (1) regardless of redshifts, stellar mass is a key parameter controlling quenching of star formation in galaxies; (2) At z<1, environmental effects become important at quenching star formation regardless of stellar mass of galaxies; and (3) However, the result of the environmental quenching is prominent only for low mass galaxies (M* < $10^{10}M_{\odot}$) since the star formation in most of high mass galaxies are already quenched at z > 1.

• Composites Research
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• 제12권6호
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• pp.65-73
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• 1999

본 연구에서는 Z-단면 복합재 스트링거의 크리플링 응력 및 파손 거동을 비선형 유한요소법을 사용하여 해석하였다. 스트링거는 9절점 쉘요소를 사용하여 이상화하였다. 취성이 강한 재료에 적합한 완전제하 모델을 사용하여 초기 파손 이후 크리플링이 발생할 때까지의 점진적 파손해석을 수행하였다. 완전제하모델을 사용한 수치적 해석을 위해 수정된 Riks방법을 도입하였다. 해석의 타당성 검증을 위해 좌굴응력 크리플링 응력을 기존 시험결과와 비교하였다. 해석결과 Z-단면 스트링거의 크리플링 응력은 플렌지의 폭이 가장 큰 영향을 미치는 것으로 나타났고,적층순서에 따라서는 $[{\pm}45/0/90]s$에서 크리플링 응력 및 부분좌굴 응력이 가장 높게 나타났다.