• 한국구조물진단유지관리공학회 논문집
• /
• 제10권2호
• /
• pp.59-67
• /
• 2006

본 연구의 목적은 면진건물의 설계를 수행하는데 있어, 면진건물의 주기, 수평 변위량 등과 같은 면진장치의 성능을 결정하기 위한 중요 요소들을 손쉽게 산정할 수 있는 포락해석용 도표를 산정하는데 있다. 이를 위하여 가속도로 표현되는 설계지진의 위험도 대신, 에너지와 관계된 $V_E$ 스펙트럼을 아울러 산정한다. UBC 97의 지진응답계수를 적용한 경계주기 $T_G$ 및 최대속도 응답 $V_0$를 지반조건별로 제안하였으며, 이를 근간으로 한 스펙트럼 작성법을 제안하였다. 제안된 $V_E$ 스펙트럼을 근거로 지반조건별 포락해석용 도표를 작성하였다.

• 천문학회지
• /
• 제26권2호
• /
• pp.115-134
• /
• 1993

The light curve and radial velocity curve of multiperiodic dwarf cepheid VI719 Cyg (HD200925) with peculiar light curve have been reanalyzed in order to identify the oscillation modes to confirm the helium settling within the envelope. To do these, through the period search for the photometric and radial velocity data from the literature, two different periods were determined and the oscillation modes corresponding to the first and second periods were identified as the fundamental and first radial overtones. Hence the helium settling within the envelope was confirmed from the period ratio. The color excess, metallicity, effective temperature, and surface gravity corresponding to two different modes were determined and it was found that these parameters almost do not depend upon different oscillation mode. By utilizing the surface brightness method, we investigated the variation of angular diameter and radial displacement and it was found that the angular variation is very peculiar. Also by referring to the stellar models, mass and age were determined as $2.7M_{\bigodot}$ and 0.42 Gyr respectively which make this variable star heavier and younger than other multimode dwarf cepheids. Preliminary spectroscopic CCD observations were carried out and it was found that Mg in VI719 Cygni is nearly solar abundent according to the analysis of $5172.68{\AA}MgI$ line which is inconsistent with the photometric result. It was suggested that VI719 Cyg may be classified as a $\rho$ Pup stars according to the photometric characteristics.

• 물과 미래
• /
• 제19권1호
• /
• pp.75-86
• /
• 1986

본연구는 하천유역에 있어서, 대규모 수공구조물의 설계홍수량 결정을 위한 최대가능강우량(PMP)분석 및 적용에 그 목적이 있다. PMP는 수문기상학적 방법,통계학적 방법, 포락선 방법으로 산정하였으며, 최대가능홍수량(PMF)은 합성단위도법과 Chow 방법으로 산정하였다. 각 방법에 의한 PMP를 비교해 본 결과, 통계학적 방법, 수문기상학적 방법, 포락선 방법의 크기 순으로 나타나고 있음을 알 수 있었으며, 산정된 PMP를 기왕의 최대강우량과 비교해 본 결과 수문기상학적 방법이 기상학적 제요소를 고려한 방법이 가장 타당한 방법이라고 사료된다. 산정된 PMP 및 PMF를 확률 수문량과 비교해 본 결과 수문기상학적 방법 및 통계학적 방법은 재현기간 1000년 확률 수문량을 다소 상회하는 것으로 나타났으며, 포락선 방법은 재현기간 200∼500 년 확률 수문량에 접근하고 있음을 알 수 있었다.대규모 수공 구조물의 설계에 있어서 위험도를 고려할 경우에는 PMP로부터 PMF를 산정하는 것이 타당할 것이다.

• 천문학논총
• /
• 제30권2호
• /
• pp.219-221
• /
• 2015

We present our recent observations of SDSS J102102.25+174439.9, a new eclipsing white dwarf - main sequence WDMS binary with an orbital period of 0.14 days. This system belongs to the post common-envelope binary group as shown by the spectrum from the Sloan Digital Sky Survey. We obtained our data using the ULTRASPEC instrument installed on the 2.4-m telescope at the Thai National Observatory (TNO). Our multi-band observations reveal an unusual and persistent drop in brightness after the primary eclipse. These dips, which appear to show variations in amplitude, also have a complex shape that changes within days. Dips in WDMS systems have been observed on only one other occasion, in the light curve of QS Vir prior to the eclipse of the white dwarf. The dips in SDSS J1021+1744 are unique because they are present at different wavelengths and they occur approximately at similar phases. Hosting a DA white dwarf and an M4 companion star, this system is known to be the only WDMS to show these kind of dips in its light curve. It is possible that these dips are caused by ejected materials from an active companion star, such as in QS Vir. The light curve in the g' filter exhibits deep and narrow features, implying that the material which passes in front of the white dwarf in SDSS J1021 must be dense and small in size. Furthermore, we try to constrain the stellar and orbital parameters of SDSS J1021+1744 using the Binary Maker 3 software. We use g' and r' data for our light curve analysis to have a better approximation for the red dwarf star.

• 한국콘크리트학회:학술대회논문집
• /
• 한국콘크리트학회 2000년도 봄 학술발표회 논문집
• /
• pp.599-604
• /
• 2000

The analytical studies for the test results are presented. From experimental envelope curve, hysteretic behaviors under cyclic loading are modelled for beam-column subassemblages. Modelled curves show relatively good reproduction or experimental curves. finally, seismic performances are investigated for 7 story plain framed structure by nonlinear dynamic analysis. The resulting responses are different by each beam-column joint design.

• 한국구조물진단유지관리공학회 논문집
• /
• 제11권3호
• /
• pp.185-191
• /
• 2007

본 연구에서는 주거용 무량판구조의 내진성능을 개선하기 위한 면진적용 가능성을 평가하였으며, 시간이력 해석을 위한 지진기록 사용에 대한 문제점을 제시하였다. 면진층 강성 및 주기 평가 및 포락해석법을 적용하여 면진전 비틀림 모드가 강한 구조물을 면진시스템 적용으로 내진성능을 개선하였다. 지진기록 사용 및 크기 조절효과의 적정성을 평가하기 위하여 DBE, MCE, ASCE 7-05의 1.4DBE 의해 크기를 조정한 시간이력 해석결과를 비교한 결과, 구조물의 지반조건과 유사한 조건에서 관측된 지진기록 및 지진기록의 응답이 설계규준 응답스펙트럼의 평균${\pm}$표준편차 범위 안에 있는 기록을 사용하는 것이 적절한 것으로 판단된다.

• 천문학회지
• /
• 제54권4호
• /
• pp.129-137
• /
• 2021

It has been established that the acoustic mode parameters of the Sun and Sun-like stars vary over activity cycles. Since the observed variations are not consistent with an activity-related origin, even Sun-like stars showing out-of-phase changes of mode frequencies and amplitudes need to be carefully studied using other observational quantities. In order to test whether the presumed relations between the global seismic parameters are a signature of the stellar activity cycle, we analyze the photometric light curve of HD 49933 for which the first direct detection of an asteroseismic signature for activity-induced variations in a Sun-like star was made, using observations by the CoRoT space telescope. We find that the amplitude of the envelope significantly anti-correlates with both the maximum frequency of the envelope and the width of the envelope unless superflare-like events completely contaminate the light curve. However, even though the photometric proxy for stellar magnetic activity appears to show relations with the global asteroseismic parameters, they are statistically insignificant. Therefore, we conclude that the global asteroseismic parameters can be utilized in cross-checking asteroseismic detections of activity-related variations in Sun-like stars, and that it is probably less secure and effective to construct a photometric magnetic activity proxy to indirectly correlate the global asteroseismic parameters. Finally, we seismically estimate the mass of HD 49933 based on our determination of the large separation of HD 49933 with evolutionary tracks computed by the MESA code and find a value of about 1.2M_☉ and a sub-solar metallicity of Z = 0.008, which agrees with the current consensus and with asteroseismic and non-asteroseismic data.

• 한국컴퓨터그래픽스학회논문지
• /
• 제7권3호
• /
• pp.1-7
• /
• 2001

본 논문에서는 canal 곡면의 투시 윤곽곡선 (perspective silhouette)에 대한 매개변수화 (parametrization) 방법과 윤곽곡선을 이루는 모든 연결된 구성요소 (connected component)를 발견하는 효율적이고 안정성 있는 알고리즘을 제시한다. Canal 곡면은 반경이 변화하면서 이동하는 구 (moving sphere)의 외곽곡면 (envelope surface)이며, 구의 중심점의 궤적을 나타내는 곡선 C(t)와 구의 반경 함수 r(t)에 의해 정의된다. 이동 구는 canal 곡면과 원에서 교차한다. Canal 곡면을 원의 집합으로 분할함으로써, 각각의 원 위에서 주어진 관측점에 대한 투시적 윤곽곡선을 구성하는 점을 계산하여 매개변수화하는 방법을 제시한다. 고정된 중심점 $C(t_*)$와 반경 $r(t_*)$를 갖는 이동 구는 canal 곡면과 하나의 원 $K(t_*)$에서 교차한다. 또한 이동 구를 관측점에서 볼 때의 윤곽곡선도 다른 하나의 원 $Q(t_*)$을 구성한다. 두 원 $K(t_*)$와 $Q(t_*)$가 한 점에서 접하게 되는 t의 값을 구함으로써 canal 곡면에 대한 윤곽곡선을 이루는 모든 연결된 구성요소를 발견하는 효율적인 방법을 제시한다.

• 대한전기학회:학술대회논문집
• /
• 대한전기학회 2011년도 제42회 하계학술대회
• /
• pp.91-92
• /
• 2011

Beat is a phenomenon, where the magnitudes and frequencies of the voltage and the current fluctuate. This paper describes a quantitative analysis of the beat phenomenon of a wind farm using the envelope of a current during intertie/grid fault conditions. In this paper, the ratio of the crest to the trough of the envelope curve and the time interval between adjacent troughs are defined and used to evaluate the beat phenomenon quantitatively. Beat phenomena under various fault and wind conditions are analyzed. The proposed quantitative analysis seems simple but effective in the more understanding of beat phenomenon of a wind farm, and thus can be used as a basis for operation and/or protection of an intertie.

• Structural Engineering and Mechanics
• /
• 제55권5호
• /
• pp.1037-1053
• /
• 2015

This paper presents finite element (FE) based pushover analysis of a reinforced concrete structure with a two-leaf cavity wall (TLCW) to estimate the performance level of this structure. In addition to this, an unreinforced masonry (URM) model was selected for comparison. Simulations and analyses of these structures were performed using the DIANA FE program. The mentioned structures were selected as two storeys and two bays. The dimensions of the structures were scaled 1:1.5 according to the Cauchy Froude similitude law. A shake table experiment was implemented on the reinforced concrete structure with the two-leaf cavity wall (TLCW) at the National Civil Engineering Laboratory (LNEC) in Lisbon, Portugal. The model that simulates URM was not experimentally studied. This structure was modelled in the same manner as the TLCW. The purpose of this virtual model is to compare the respective performances. Two nonlinear analyses were performed and compared with the experimental test results. These analyses were carried out in two phases. The research addresses first the analysis of a structure with only reinforced concrete elements, and secondly the analysis of the same structure with reinforced concrete elements and infill walls. Both researches consider static loading and pushover analysis. The experimental pushover curve was plotted by the envelope of the experimental curve obtained on the basis of the shake table records. Crack patterns, failure modes and performance curves were plotted for both models. Finally, results were evaluated on the basis of the current regulation ASCE/SEI 41-06.