• Structural Engineering and Mechanics
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• 제73권3호
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• pp.271-286
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• 2020

Passive control technologies are commonly used in several areas to suppress structural vibrations by the addition of supplementary damping, and some modal damping may be heavy beyond critical damping even for regular structures with energy dissipation devices. The design of passive control structures is typically based on (complex) mode superposition approaches. However, the conventional mode superposition approach is predominantly applied to cases of under-critical damping. Moreover, when any modal damping ratio is equal or close to 1.0, the system becomes defective, i.e., a complete set of eigenvectors cannot be obtained such that some well-known algorithms for the quadratic eigenvalue problem are invalid. In this paper, a generalized complex mode superposition method that is suitable for under-critical, critical and over-critical damping is proposed and expressed in a unified form for structural displacement, velocity and acceleration responses. In the new method, the conventional algorithm for the eigenvalue problem is still valid, even though the system becomes defective due to critical modal damping. Based on the modal truncation error analysis, modal corrected methods for displacement and acceleration responses are developed to approximately consider the contribution of the truncated higher modes. Finally, the implementation of the proposed methods is presented through two numerical examples, and the effectiveness is investigated. The results also show that over-critically damped modes have a significant impact on structural responses. This study is a development of the original complex mode superposition method and can be applied well to dynamic analyses of non-classically damped systems.

• 천문학논총
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• 제32권1호
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• pp.239-244
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• 2017

How does the presence of an AGN influence the total SFR estimates of galaxies and change their distribution with respect to the Galaxy Main Sequence? To contribute to solving this question, we study a sample of 1133 sources detected in the North Ecliptic Pole field (NEP) by AKARI and Herschel. We create a multi-wavelength dataset for these galaxies and we fit their multi-wavelength Spectral Energy Distribution (SED) using the whole spectral regime (from 0.1 to $500{\mu}m$). We perform the fit using three procedures: LePhare and two optimised codes for identifying AGN tracers from the SED analysis. In this work we present an overview of the comparison between the estimates of the Infrared bolometric luminosities (between 8 and $1000{\mu}m$) and the AGN fractions obtained exploiting these different procedures. In particular, by estimating the AGN contribution in four different wavelength ranges ($5-40{\mu}m$, $10-20{\mu}m$, $20-40{\mu}m$ and $8-1000{\mu}m$) we show how the presence of an AGN affects the PAH emission by suppressing the ratio $\frac{L_{8{\mu}m}}{L_{4.5{\mu}m}}$ as a function of the considered wavelength range.

• 대한화학회지
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• 제32권1호
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• pp.9-14
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• 1988

$La_{1-x}Ca_xFeO_{3-y}$ 계의 perovskite 형의 화합물은 La_2O_3,\;CaCO_3$, 및 Fe(NO-3)_3{\cdot}9H_2O$의 정량적 혼합물은 1100$^{\circ}C$에서 24시간 동안 가열하여 제조하였다. 이 고용체의 결정구조는 모든 조성에서 사방정계였다. X-선 회절분석과 Mohr 염 분석을 통하여 y값이 증가하면 공위배열에 의한 상전이가 일어나며 격자체적은 x값이 증가함에 따라 감소한다는 것을 확인하였다. 비화학양론적 조성 y는 0.0에서 0.5사이의 값을 나타내었다. Mossbauer 분광분석을 298K에서 수행하여 x = 0.75 조성이 높은 닐온도를 갖는다는 것을 확인하였다. 시료의 전기전도도는 $-100{\sim}100^{\circ}C$ 온도범위에서 측정하였다. 활성화 에너지로부터 공위 배열에 기인한 열린 통로를 갖고 있는 시료들은 이온성 전기전도에 의한 기여가 어느 정도 존재하는 것으로 밝혀졌다.

• Bulletin of the Korean Chemical Society
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• 제34권3호
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• pp.810-814
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• 2013

The thermodynamic parameters for the intercalative interaction of structurally related well known intercalators, 9-aminoacridine (9AA) and proflavine (PF) were determined by means of fluorescence quenching study. The fluorescence intensity of 9AA decreased upon intercalation to DNA, poly[$d(A-T)_2$] and poly[$d(G-C)_2$]. A van't Hoff plot was constructed from the temperature-dependence of slope of the ratio of the fluorophore in the absence and presence of a quencher molecule with respect to the quencher concentration, which is known as a Stern-Volmer plot. Consequently, the thermodynamic parameters, enthalpy and entropy change, for complex formation was calculated from the slope and y-intercept of the van't Hoff plot. The detailed thermodynamic profile has been elucidated the exothermic nature of complex formation. The complex formation of 9AA with DNA, poly[$d(A-T)_2$] and poly[$d(G-C)_2$] was energetically favorable with a similar negative Gibb's free energy. On the other hand, the entropy change appeared to be unfavorable for 9AA-poly[$d(G-C)_2$] complex formation, which was in contrast to that observed with native DNA and poly[$d(A-T)_2$] cases. The equilibrium constant for the intercalation of PF to poly[$d(G-C)_2$] was larger than that to DNA, and was the largest among sets tested despite the most unfavorable entropy change, which was compensated for by the largest favorable enthalpy. The favorable hydrogen bond contribution to the formation of the complexes was revealed from the analyzed thermodynamic data.

• 천문학회보
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• 제39권2호
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• pp.74.1-74.1
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• 2014

We study a wraping instability of a geometrically thin, non-self-gravitating disk surrounding binary supermassive black holes on a circular orbit. Such a circumbinay disk is subject to not only tidal torques due Line 8 to the binary gravitational potential but also radiative rorques due to radiation emitted from each accretion disk. We find tat a circumbinary disk initially aligned with the binary orbital plane is unstable to radiation-driven warping beyond the marginally stable warping radius, which is sensitive to both the ratio of vertical to horizontal shear viscosities and the mass-to-energy conversion efficiency. As expected, the tidal torques give no contribution to the growth of warping modes but tend to align the circumbinary disk with the orbital plane. Since the tidal torques can suppress the warping modes in the inner part of circumbinary disk, the circumbinaary disk starts to be warped at the radii larger than the marginally stable warping radius. If the warping radius is of the order of 0.1 pc, a resultant semi-major axis is estimated to be of the order of 10-2 pc to 10-4 pc for 107 Msun black hole. We also discuss the posibility that the central objects of observed warped maser disks in active galactic nuclei are binary supermassive black holes with a triple disk: two accretion disks around the individual black holes and one circumbinary disk surrounding them.

• 한국생활과학회지
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• 제8권3호
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• pp.477-486
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• 1999

This study was performed to investigate the variation in dietary fiber and fat intakes, and the contribution of food groups to dietary fiber and fat consumption in relation to age and to examine the relationship between dietary fiber and fat intakes in 337 urban adults aged 20-49 year. Dietary intakes were evaluated with one-day 24-hour recall and two-day dietary record method. Significantly higher intakes of fat in males and saturated fatty acid, monounsaturated fatty acid, polyunsaturated fatty acid, and cholesterol in females were associated with younger age. The ratio of fat to the total energy intake slightly exceeded 20% at 20s and 30s in both males and females. The main source of dietary fiber was vegetables in all age groups of males and 30s of females, but grains in 20s and 40s of females. The main source of fat was meats in all age groups of males and 40s of females, but grains in 20s and 30s in females. The main source of cholesterol was eggs in both males and females. Dietary fiber intake was positively correlated with all fat-related parameters except cholesterol in 20s and 40s and was positively related with fat in 30s of males. For females dietary fiber intake was positively correlated with polyunsaturated fatty acid in 20s and with monounsaturated fatty acid and polyunsaturated fatty acid in 40s. These findings show that there is considerable variation in intake of dietary fiber and fat in relation to age among adults and suggest that these factors should be considered at interventions aimed toward improvement of nutritional status.

• 한국가스학회지
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• 제11권4호
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• pp.17-22
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• 2007

비예혼합 대향류화염에서 산소부화에 따른 NOx 생성특성에 관한 수치해석이 수행되었다. 순산소의 연소과정에서 공기침투에 의한 부득이한 질소 유입의 상황을 체계적으로 고려하기 위하여, 산화제의 $O_2$는 체적비 21%에서 100%까지 변화되었다. 결과적으로 NO 배출지수$(EI_{NO})$는 산소부화율 75%까지 증가하다가 급격히 감소하는 경향을 보여준다. 이러한 경향은 화염온도, 화염두께 및 체류시간 보다는 NOx 생성과 관련된 $N_2$ 소모율 변화에 의해 설명될 수 있음을 확인하였으며, 특히 N+NO=$N_2+O$ 반응이 가장 크게 기여함을 알 수 있었다.

• Advances in concrete construction
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• 제12권5호
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• pp.377-389
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• 2021

Reinforced concrete vertical silos are universal structures that store large amounts of granular materials. Due to the asymmetric structure, heavy load, uneven storage material distribution, and the difference between the storage volume and the storage material bulk density, the corresponding earthquake is very complicated. Some scholars have proposed the calculation method of horizontal forces on reinforced concrete vertical silos under the action of earthquakes. Without considering the effect of torsional effect, this article aims to reveal the expansion factor of the silo group considering the torsional effect through experiments. Through two-way seismic simulation shaking table tests on reinforced concrete column-supported group silo structures, the basic dynamic characteristics of the structure under earthquake are obtained. Taking into account the torsional response, the structure has three types of storage: empty, half and full. A comprehensive analysis of the internal force conditions under the material conditions shows that: the different positions of the group bin model are different, the side bin displacement produces a displacement difference, and a torsional effect occurs; as the mass of the material increases, the structure's natural vibration frequency decreases and the damping ratio Increase; it shows that the storage material plays a role in reducing energy consumption of the model structure, and the contribution value is related to the stiffness difference in different directions of the model itself, providing data reference for other researchers; analyzing and calculating the model stiffness and calculating the internal force of the earthquake. As the horizontal side shift increases in the later period, the torsional effect of the group silo increases, and the shear force at the bottom of the column increases. It is recommended to consider the effect of the torsional effect, and the increase factor of the torsional effect is about 1.15. It can provide a reference for the structural safety design of column-supported silos.

• 환경영향평가
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• 제27권1호
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• pp.56-72
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• 2018

북한은 환경자원 소비가 충분하지 못함에도 불구하고 생태발자국이 생태수용력보다 큰 생태적자 상태이다. 본 연구에서는 북한의 생태수용력과 생태발자국, 생태적자 추이를 살펴보고, 생태발자국과 생태수용력의 비를 의미하는 오버슈트 비율에 영향을 준 5개 요인의 기여도를 살펴보았다. 5개 요인은 생태발자국을 구성하는 인구와 개인의 환경자원 소비강도를 의미하는 일인당 생태발자국, 생태수용력을 구성하는 토지면적, 생산성인자, 그리고 토지면적과 생산성인자를 제외하고 생태수용력에 영향을 주는 요인(등가인자와 연간생산성인자 변화율의 곱)이다. 북한의 생태적자는 생태수용력보다 생태발자국을 구성하는 요인에 의한 기여가 높았다. 생태적자는 1966년에 시작되었는데, 이 시점부터 1990년대 중반까지는 일인당 생태발자국 값이 오버슈트 비율에 기여하는 비율이 60% 전후로 가장 높았고, 1990년대 중반 이후에는 인구에 의한 기여도가 40~60%로 가장 높았다. 토지면적과 생산성인자에 의한 기여도도 1990년대 중반 이후 높아져서 토지면적은 최대 15%, 생산성인자는 최대 18%까지 증가하였다. 생태수용력과 생태발자국 모두에서 높은 비중을 차지한 경작지 부문의 경우, 면적이 증가했음에도 불구하고 생산성이 줄어들어 생태수용력이 감소하였다. 북한의 생태적자를 줄이기 위해서는 1990년 이후 눈에 띄게 줄어들고 있는 산림면적을 이전 수준으로 복구하고, 경작지의 생산성을 높이기 위한 방안을 마련해야 할 것이다. 또한 근본적으로 북한 주민의 빈곤을 해결할 수 있는 식량 지원 방안, 자연재해에 대한 취약성을 극복할 수 있는 방안도 함께 마련되어야 할 것이다.

• Journal of Nutrition and Health
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• 제41권6호
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• pp.530-538
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• 2008

초등학생들의 음료수 섭취실태를 살펴보고 우유 및 가당 음료수섭취가 아동들의 영양소섭취와 비만도에 미치는 영향을 알아보기 위해 경남의 초등학생 160명을 대상으로 2006년 6월부터 7월까지 신체계측을 실시하고, 정량적 빈도법을 이용하여 음료수섭취량을 조사하였다. 또 24시간 회상법을 사용하여 비연속적으로 3일간의 영양소섭취량을 조사하였다. 조사대상 아동들의 음료수의 총 섭취빈도는 1개월에 93.5회로 하루 평균 3.1회 정도였다. 음료수 중, 우유섭취빈도가 가장 높았는데 1개월에 36회로 하루 평균 1회 이상 우유를 섭취하였으며 다음으로 주스, 발효유, 탄산음료의 순이었다. 또 총 음료수 섭취량은 하루 평균 626.6 mL였고, 이 중 우유를 가장 많이 섭취하였고(253.8 mL), 다음으로 주스(133.6 mL), 탄산음료(77.7 mL)의 순이었다. 또 우유와 두유를 제외한 가당 음료수 섭취량은 359.7 mL였다. 전체 음료수 섭취열량은 328.5 kcal로, 하루 섭취열량의 20.3%였으며, 우유 및 두유로부터 섭취한 열량은 하루 섭취열량의 9.8%였고, 가당 음료는 10.5%였다. 남녀 아동별로 비교해 보았을 때 가당 음료로부터 얻는 열량의 비율이 여자가 13.5%, 남자가 7.7%로 여자가 남자에 비해 유의하게 높았다. 가당 음료수를 섭취하는 빈도와 이로 부터 얻는 열량이 높을수록 단백질, 비타민 A, 나이아신의 섭취량이 낮아서 아동들의 식사의 질이 낮았을 가능성이 있었다. 그러나 우유 및 두유 섭취빈도는 아동들의 영양섭취와 상관이 없었다. 우유 및 두유 섭취빈도가 높을 수록 키는 컸고, 체지방비와 WHR은 낮았으며 우유 및 두유섭취량이 많을수록, 체지방비와 WHR은 낮았다. 또 우유 및 두유로 부터의 섭취열량이 많을수록 WHR은 낮았지만, 가당 음료수 섭취는 신체계측치와 상관이 없었다. 결론적으로 초등학생들의 경우 우유 및 두유 섭취빈도는 아동들의 영양소섭취와 상관이 없었고, 우유 및 두유섭취량이 많을수록 체지방비와 WKR은 낮았다. 반면에 가당 음료수 섭취가 영양적인 측면에서 식사의 질을 저하시킬 가능성은 있었지만, 아동의 비만도와는 관련이 없었다.