• 한국재료학회지
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• 제22권9호
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• pp.482-488
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• 2012

To fabricate a precise micro metal mold, the electrochemical etching process has been researched. We investigated the electrochemical etching process numerically and experimentally to determine the etching tendency of the process, focusing on the current density, which is a major parameter of the process. The finite element method, a kind of numerical analysis, was used to determine the current density distribution on the workpiece. Stainless steel(SS304) substrate with various sized square and circular array patterns as an anode and copper(Cu) plate as a cathode were used for the electrochemical experiments. A mixture of $H_2SO_4$, $H_3PO_4$, and DIW was used as an electrolyte. In this paper, comparison of the results from the experiment and the numerical simulation is presented, including the current density distribution and line profile from the simulation, and the etching profile and surface morphology from the experiment. Etching profile and surface morphology were characterized using a 3D-profiler and FE-SEM measurement. From a comparison of the data, it was confirmed that the current density distribution and the line profile of the simulation were similar to the surface morphology and the etching profile of the experiment, respectively. The current density is more concentrated at the vertex of the square pattern and circumference of the circular pattern. And, the depth of the etched area is proportional to the current density.

• 문화기술의 융합
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• 제9권6호
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• pp.919-925
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• 2023

현대의 드론에 장착되고 있는 임무 장비들의 소형화되고, 감시, 정찰 등의 여러 임무를 수행한다. 이에 따라 임무 장비는 풍하중, 모터 회전 등에 외란에 노출이 되어있으며, EOTS 구동에 있어 불안정성을 야기할 수 있다. 특히 EOTS의 시선의 위치 변경에 있어 단순 Step 입력은 급격한 속도의 변화를 일으켜 오버슈트를 발생시키며 여러 외란과 함께 불안정성을 야기할 수 있다. 따라서 EOTS의 시선의 변경을 할 시에 각속도가 사다리꼴 형태로 움직일 수 있도록 프로파일을 설정하고, 이를 이중 루프 제어기를 설계하여 위치 피드백을 받는 외부 루프의 Input에 적용 후 시스템의 안정성 비교와 최대 속도, 최대 가속도를 변화시키면서, 시스템이 안정적인 범위 내에서 속도 프로파일의 최적화를 연구하였다.

• 한국지구과학회지
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• 제35권7호
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• pp.529-536
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• 2014

이 논문에서는 한 개의 측선에서 측정된 중력 변화율 텐서를 이용하여 선형 이상체의 주향과 경사를 자동 결정하는 알고리즘을 제시한다. 선형 이상체의 중력 변화율은 측선에 수직으로 배열되어 있는 경우 이차원 효과를 보이므로, 이론적으로 두 개의 독립 성분을 제외하고는 값을 갖지 아니한다. 반면 주향과 경사를 가지는 선형 이상체는 5개의 독립 성분을 가지게 된다. 이와 같은 선형 이상체가 가지는 중력 변화율 텐서의 이차원 특성을 활용하여 5개의 독립 성분 중 3개가 동시에 최소 값이 되도록 하는 회전변환의 변환각은 곧바로 선형 이상체의 주향과 경사를 의미한다. 이 논문에서는 최소자승법을 이용하여 5개의 중력 변화율 성분 중 3개를 최소로 하는 변환 행렬 각을 구하였고 이를 이용하여 선형 이상체의 주향과 경사를 자동 결정할 수 있음을 보였다. 이 논문에서는 모델 계산을 통하여 주향만 있는 경우와 주향과 경사 모두를 가지는 경우에 대하여 각각의 방향각들을 자동 결정할 수 있음을 보였다.

• 천문학회지
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• 제54권5호
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• pp.139-155
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• 2021

We present an updated version of the multilayer spectral inversion (MLSI) recently proposed as a technique to infer the physical parameters of plasmas in the solar chromosphere from a strong absorption line. In the original MLSI, the absorption profile was constant over each layer of the chromosphere, whereas the source function was allowed to vary with optical depth. In our updated MLSI, the absorption profile is allowed to vary with optical depth in each layer and kept continuous at the interface of two adjacent layers. We also propose a new set of physical requirements for the parameters useful in the constrained model fitting. We apply this updated MLSI to two sets of Hα and Ca II line spectral data taken by the Fast Imaging Solar Spectrograph (FISS) from a quiet region and an active region, respectively. We find that the new version of the MLSI satisfactorily fits most of the observed line profiles of various features, including a network feature, an internetwork feature, a mottle feature in a quiet region, and a plage feature, a superpenumbral fibril, an umbral feature, and a fast downflow feature in an active region. The MLSI can also yield physically reasonable estimates of hydrogen temperature and nonthermal speed as well as Doppler velocities at different atmospheric levels. We conclude that the MLSI is a very useful tool to analyze the Hα line and the Ca II 8542 line spectral daya, and will promote the investigation of physical processes occurring in the solar photosphere and chromosphere.

• 천문학회지
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• 제29권spc1호
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• pp.263-264
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• 1996

We have solved the radiative transfer problem using a Sobolev approximation with an escape probability method in case of the supersonic expansion of a stellar envelope to an ambient medium. The radiation from the expanding envelope turns out to produce a P-Cygni type profile. In order to investigate the morphology of the theoretical P-Cygni type profile, we have treated $V{\infty},\;V_{sto},\;{\beta}$ (parameter for the velocity field), M and $\epsilon$ (parameter for collisional effect) as model parametrs. We have found that the velocity field and the mass loss rate affect the shapes of the P-Cygni type profiles most effectively. The secondarily important factors are $V{\infty},\;V_{sto}$. The collisional effect tends to make the total flux increase but not so .much in magnitude. We have infered some physical parameters of 68 Cyg, HD24912, and $\xi$ persei such as V$\infty$, M from the model calculation, which shows a good agreement with the observational results.

• 한국지진공학회논문집
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• 제9권6호
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• pp.67-73
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• 2005

엄밀한 지반-구조물 상호작용 해석을 위해서는 지반에 대한 묘사가 적절히 이루어져야 한다. 그러나 물성이 불연속적이거나 지층의 모양이 복잡할 때에는 유한요소망을 구성하는 것이 어려운데, 그 이유는 유한요소망이 지층의 모양을 정확히 나타내어야하기 때문이다. 이러한 어려움을 극복하기 위하여 본 연구에서는 지층의 불연속선을 따라 요소를 재배열하지 않고 엄밀하게 수치적분이 가능한 방법을 채용하였다. 그 결과로 정렬된 요소망을 그대로 이용하게 되어 강성행렬의 성질이 좋아지며, 해석 또한 신뢰성이 높아지게 되었다. 이 해석 방법을 이용하여 지진응답에 미지는 지층의 영향을 조사하였으며, 결과적으로 복잡하고 불연속적인 물성을 가지는 지층으로 이루어진 지반과 구조물의 상호작용을 해석하는 데에 쉽게 이용 될 수 있음을 보였다.

• 한국전산유체공학회:학술대회논문집
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• 한국전산유체공학회 2008년도 춘계학술대회논문집
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• pp.420-423
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• 2008

This present work is to find optimum design of a NACA65 axial fan blade with weighted average surrogate model. The numerical analysis by Reynolds-average Navier-Stokes equations with shear stress turbulence(SST) is discretized by finite volume approximations and solved on hexahedral grids for flow analysis. The blade aerodynamic shape is modified by six design variables for the optimization. The blade profile as well as stacking line is modified to enhance blade total efficiency. Six design variables, airfoil maximum camber, maximum camber location, leading edge radius, trailing edge radius, lean angle at 50% span and lean angle at 100% span, are selected for blade profile to enhance the total efficiency. The PBA model which is basically weighted average of the basis surrogates is used to find the optimal design in the design space from the constructed response surface model for the objective function. By the optimization, the total efficiency is increased by 1.4%.

• 천문학회보
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• 제46권1호
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• pp.32.3-33
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• 2021

We present H I gas kinematics and star formation activities of NGC 6822, a dwarf galaxy located in the Local Volume at a distance of ~ 490 kpc. We perform profile decomposition of the line-of-sight velocity profiles of the high-resolution (42.4" × 12" spatial; 1.6 km/s spectral) H I data cube taken with the Australia Telescope Compact Array (ATCA). For this, we use a new tool, the so-called BAYGAUD (BAYesian GAUssian Decompositor) which is based on Bayesian Markov Chain Monte Carlo (MCMC) techniques, allowing us to decompose a line-of-sight velocity profile into an optimal number of Gaussian components in a quantitative manner. We classify the decomposed H I gas components of NGC 6822 into bulk-narrow, bulk-broad, and non_bulk with respect to their velocity and velocity dispersion. We correlate their gas surface densities with the surface star formation rates derived using both GALEX far-ultraviolet and WISE 22 micron data to examine the impact of gas turbulence caused by stellar feedback on the Kennicutt-Schmidt (K-S) law. The bulk-narrow component that resides within r25 is likely to follow the linear extension of the Kennicutt-Schmidt (K-S) law for molecular hydrogen (H2) at the low gas surface density regime where H I is not saturated.

• 천문학회지
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• 제29권2호
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• pp.93-105
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• 1996

We have solved the radiative transfer problem using a Sobolev approximation with an escape probability method in case of the supersonic expansion of a stellar envelope to an ambient medium. The radiation from the expanding envelope turns out to produce a P-Cygni type profile. In order to investigate the morphology of the theoretical P-Cygni type profile, we have treated $V_\infty,\;V_{sto},\;\beta$ (parameters for the velocity field), it and E(parameter for collisional effect) as model parameters. We have investigated that the velocity field and the mass loss rate affect the shapes of the P-Cygni type profiles most effectively. The secondarily important factors are $V_\infty,\;V_{sto}$. The collisional effect tends to make the total flux increased but not so much in magnitude. We have infered some physical parameters of 68 Cyg, HD24912, and $\xi$ persei such as $V_\infty,\;M$ from the model calculation, which shows a good agreenment with the observational results.

• 동력기계공학회지
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• 제1권1호
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• pp.42-51
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• 1997

In this study, in order to investigate the influence of cam profile on the injection rate, the characteristics of injection in PLN (pump - line - nozzle) diesel injection system were simulated. Six types of the profile of fuel cam were used for simulation. The maximum injection pressure and maximum injection rate of initial and end phase were analyzed to demonstrate the characteristics of injection. The mathematical model of the injection system and the computation results were verified by experimental results. Simulation results showed that the maximum injection pressure, maximum injection rate, injection quantity and pressure drop in the end phase were proportional to the velocity of fuel cam during the effective stroke.