• 대기
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• 제18권3호
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• pp.159-169
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• 2008

The characteristics of the typhoon's extratropical transition (ET) over the western North Pacific area were investigated using the cyclone phase space (CPS) diagram method suggested by Hart (2003). The data used in this study were the global data assimilation prediction system (GDAPS) and NCEP data set. The number of typhoons selected were 75 cases during 2002 to 2007, and the three parameters were analyzed : the motion relative thickness asymmetry of the storm (B), the upper thermal wind shear and the lower thermal wind shear. Comparing the best-track data provided by the Regional Specialized Meteorological Center /Tokyo, the time of the ET based on CPS was 2~6 hours earlier than the best-track data. And it was shown that the 400- km and 30 kt wind radius of storm for the CPS method were better agreement than the previous suggested radius 500- km.

• 지질공학
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• 제24권4호
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• pp.643-648
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• 2014

터널의 굴착과정에서 막장전반부에 분포하는 절리를 예측하여 그들로 인한 붕괴를 예방하기위해 보강계획을 수립하는 것은 매우 중요한 사안이다. 그러나 빠른 굴착공정에서 절리의 분포를 충분히 조사하고 예측하는 것은 쉽지 않은 일이다. 본 연구는 굴착면 선단부에 분포하는 절리를 예측할 수 있는 새로운 통계적 기법을 제시하고자 한다. 제시될 방법은 단일 절리군에 대한 절리간격의 누적분포도를 이용한 절리분포의 예측이다. 누적분포도는 수평축에 절리를 동일간격으로 순차적 배열을 한 후, 수직축에 누적간격을 기준으로 각 절리를 하나의 점으로 표기한다. 이 도표에서, 표기된 점들이 선형을 이루면 절리의 분포양상이 규칙적임을 의미하며, 직선의 기울기는 절리의 간격을 의미한다. 기울기가 낮으면 절리사이의 간격이 적은 것 이다. 점들의 분포가 군집형을 이루면 이는 절리의 분포양상이 군집형을 이룸을 의미한다. 현장에서 조사된 자료를 누적분포도에 점기하면 특정 절리군에 대한 분포양상이 분포도에 표기될 것이고, 이 분포양상을 연장하면 앞으로 굴착될 굴착면 전방의 절리분포를 예측할 수 있을 것이다. 실 터널현장에서 10 m 간격에서 측정된 특정 절리군에 대한 누적분포도 분석이 수행되었으며 이를 기반으로 3 m 전방의 미 굴착구간에 대한 절리분포가 예측되었다. 예측결과를 실제 현장자료와 비교한 결과 누적분포도는 전방절리를 적절히 예측하고 있었다. 분포도의 특성상 점기된 절리들의 선형과 등간격의 군집형태는 그 자체로 절리의 분포가 규칙적이며 누적분포도의 예측이 정확할 수 있음을 의미하는 것이다. 그러므로 본 연구는 향후 누적분포도의 분포양상에 대한 고찰과 그 결과의 넓은 공유가 있기를 바란다.

• 천문학회보
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• 제42권1호
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• pp.44.4-45
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• 2017

We report the first detection of RR Lyrae variable stars in the Crater II dwarf galaxy, a recently discovered ultra-faint satellite of the Milky Way. Based on B, V time series photometry obtained with the Korea Microlensing Telescope Network (KMTNet) at CTIO, Chile, we have identified ~45 fundamental-mode (ab-type) and ~2 first-overtone (c-type) RR Lyrae stars by adopting template light-curve fitting method. Our preliminary analysis suggests an Oosterhoff-intermediate classification of this galaxy from the mean period of the RRab stars, <$P_{ab}$> ${\simeq}0.63$ days, and the location of them on the period-amplitude diagram. We discuss the properties of the RR Lyare stars in this galaxy.

• Journal of Power Electronics
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• 제14권5호
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• pp.937-945
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• 2014

This paper presents an optimized space vector pulse-width modulation (OSVPWM) technique for a five-level cascaded H-bridge (CHB) inverter. The space vector diagram of the five-level CHB inverter is optimized by resolving it into inner and outer two-level space vector hexagons. Unlike conventional space vector topology, the proposed technique significantly reduces the involved computational time and efforts without compromising the performance of the five-level CHB inverter. A further optimized (FOSVPWM) technique is also presented in this paper, which significantly reduces the complexity and computational efforts. The developed techniques are verified through MATLAB/SIMULINK. Results are compared with sinusoidal pulse-width modulation (SPWM) to prove the validity of the proposed technique. The proposed simulation system is realized by using an XC3S400 field-programmable gate array from Xilinx, Inc. The experiment results are then presented for verification.

• 한국항공우주학회지
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• 제37권4호
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• pp.359-366
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• 2009

자동 코드생성이란 MATLAB의 Simulink 환경에서 설계한 블록 다이어그램을 c 코드로 변환시켜 주는 기능으로 MATLAB과의 연동을 통해 소프트웨어 설계부터 검증까지의 통합된 개발환경을 제공함으로서 개발 시간을 크게 줄일 수 있다. 하지만 생성된 c 프로그램을 무인기에 탑재하기 위해서는 소프트웨어의 신뢰성 확보가 필요하며 특히 원본이 되는 Simulink 블록의 검증이 중요하다. 본 연구에서는 자동 코드생성 기능을 고려하여 Simulink 환경에서 구성한 무인기용 자동비행 프로그램을 DO-178B에 명시된 소프트웨어 시험 과정에 따라 검증하였다. 이 과정을 통해 최종 프로그램은 기능 요구사항에 대한 만족함을 확인했을 뿐 아니라 Decision Coverage 93%, Condition Coverage 95% 그리고 MC/DC 90%로 구조적 측면에서 검증을 수행했다.

• 한국자동차공학회논문집
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• 제6권4호
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• pp.66-75
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• 1998

In many case of optimal design and sensitivity analysis, obtaining of transfer function between input and output variables is a difficult and time-consuming problem. The bond graph modeling is a method that is used for making it easy to analyze complex systems composed of mechanical and electrical parts. It gives us a simple and systematic tool to get state-space equations easily. And we can obtain the transfer function graphically using bond graph and Mason's rule. This paper shows how bond graphs are converted to block diagram and how Mason's rule is applied. And the simple direct method to obtain transfer function from bond graph is introduced. As a example, induction of transfer function of electric power steering composed of mechanical and electrical parts will be done.

• 한국항공운항학회지
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• 제13권3호
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• pp.34-42
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• 2005

The objectives of the study are to present simple physical and mathematical models of liquid fuel in the tank of an aerospace vehicle such launch vehicle or missile and to investigate its dynamic stability for a parameter space. In this paper, liquid in the container is modeled as multi-mass system subject to parametric excitations, and a stability diagram for determination of stable-unstable regions of the motion is obtained by using an analytical method. Also, computer simulations are conducted at various parameter points to verify the analytical results, and time histories of motion are compared to explain the effect of variation of parameters of the system.

• Journal of Astronomy and Space Sciences
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• 제16권2호
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• pp.167-176
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• 1999

The optimal initial inclination for minimizing the variation of the Local Time of Ascending Node(LTAN) during the three year mission of the KOMPSAT is investigated. At first, the analytical equation for the inclination change by the Sun is derived and the optimal initial inclination by analytical method is derived. Then the analytically derived optimal inclination is checked by the numerical orbit propagation with including all major perturbations. Four different cases of the initial orbital elements are used for monitoring the LTAN variation of the LTAN. Therefore, a new optimal initial inclination by numerical orbit propagation for the KOMPSAT is found. In addition, the variations of the mean and osculating semi-major axis are investigated with the different atmospheric density values. The mean eccentricity vs. argument of perigee diagram for the frozen orbit is obtained.

• 천문학회보
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• 제38권2호
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• pp.64.1-64.1
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• 2013

High energy photons and mechanical energy produced by the process of star formation result in copious FIR molecular and atomic lines, which are important coolants of the system. Photons thermally or mechanically induced could dissociate water in the dense envelope to change relative abundances among the species O, OH, and H2O. Here we analyze OH emission lines toward embedded young stellar objects (YSOs) observed as part of the Herschel open time key program, 'Dust, Ice, and Gas In Time (DIGIT)' in order to study the physical conditions of associated gas and the energy budget loaded on the OH line emission. According to our analysis of the Herschel/PACS spectra, OH emission peaks at the central spaxel in most of sources, but several sources show spatially extended emission structures. In the extended emission sources, the distribution of OH emission is correlated with that of [OI] emission and extended along the outflow directions. Considering the diversity of source properties, ratios between detected OH lines are relatively constant among sources. In addition, each OH line has strong correlation with bolometric luminosity. For detail analyses with rotation diagram and non-LTE LVG model, we present the results from GSS30-IRS1 and Elias29.

• Journal of Astronomy and Space Sciences
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• 제36권2호
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• pp.75-86
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• 2019

UV Psc is a typical RS CVn type system undergoing dynamic chromosphere activity. We performed photometric observations of the system in 2015 and secured new BVR light curves showing well-defined photometric waves. In this paper, we analyzed the light curves using Wilson-Devinney binary code and investigated the orbital period of the system. The combination of our light curve synthesis with the spectroscopic solution developed by previous investigators yielded the absolute parameters as: $M_1=1.104{\pm}0.042M_{\odot}$, $R_1=1.165{\pm}0.025R_{\odot}$, and $L_1=1.361{\pm} 0.041L_{\odot}$ for the primary star, and $M_2=0.809{\pm}0.082M_{\odot}$, $R_2=0.858{\pm}0.018R_{\odot}$, and $L_2=0.339 {\pm}0.010L_{\odot}$ for the secondary star. The eclipse timing diagram for accurate CCD and photoelectric timings showed that the orbital period may vary either in a downward parabolic manner or a quasi-sinusoidal pattern. If the latter is adopted as a probable pattern for the period change, a more plausible account for the cyclic variation may be the light time effect caused by a circumbinary object rather than an Applegate-mechanism occurring via variable surface magnetic field strengths.