• 한국정보통신학회논문지
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• 제11권5호
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• pp.882-888
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• 2007

본 논문은 Water Shed 알고리듬을 이용하여 여러 공들 중에 숨어있는 공을 찾는 것으로써 실재 적인 목적은 Water Shed 알고리듬의 한계를 집어보고 분석해 보고자 함이다. 이로써 세포 분석이나 농산물 관련된 분야에서 사용되던 기존의 Water Shed의 문제점을 보완하는 계기가 될 것이다. 본 연구는 Visual Studio C++을 사용하여 구현해 보았으며, Distance Transform 및 Labelling 등의 알고리듬이 추가로 사용되었다.

• Journal of Astronomy and Space Sciences
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• 제16권1호
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• pp.21-30
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• 1999

소백산 천문대에서 1997년 2월부터 1998년 3월까지 총 3일 밤 동안 VRI 필터를 가지고 AK Her에 대한 CCD 측광관측을 수행하여 얻은 관측점의 수는 V는 236점, R은 198점, I는 197점이다. 관측 기간 동안 주극심과 부극심 시각을 각각 1개씩 관측하였으며, 우리의 관측자료를 가지고 VRI 광도곡선과 (O-C)도를 만들었다. Wilson-Devinney 방법으로 우리의 광도곡선을 분석한 결과 AK Her는 접촉형 (모드 3)의 경우는 해를 구할 수 없었고, 나머지(모드2, 4, 5)에 대해서는 접촉형에 가까운 분리형 또는 반분리형이라고 할 수 있었다. 우리의 최근자료를 가지고 만든 (O-C)도에서 AK Her 공전주기는 Borkovits & Hegedus의 예상과는 다르게 1990년도 이후 증가하는 변화가 나타났다.

• Bulletin of the Korean Chemical Society
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• 제14권1호
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• pp.101-107
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• 1993

Ab initio calculations are carried out at the 6-311G$^{**}$ level for the $C_{2v}$ interactions of Be and Li atoms with acetylene molecule. The main contribution to the deep minima on the $^3B_2\;BeC_2H_2\;and\;^2B_2 LiC_2H_2$ potential energy curves is the b_2\;(2p(3b_2)-l{\pi}_g^*(4b_2))$ interaction, the $a_1\;(2s(6a_1)-I{\pi}_u(5a_1))$ interaction playing a relatively minor role. The exo deflection of the C-H bonds is basically favored, as in the $b_2$ interaction, due to steric crowding between the metal and H atoms, but the strong in-phase orbital interaction, or mixing, of the $a_1$ symmetry hydrogen orbital with the $5a'_1,\;6a'_1,\;and\;7a'_1$ orbitals can cause a small endo deflection in the repulsive complexes. The Be complex is more stable than the Li complex due to the double occupancy of the 2s orbital in Be. The stability and structure of the $MC_2H_2$ complexes are in general determined by the occupancy of the singly occupied frontier orbitals.

• 한국재료학회지
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• 제2권3호
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• pp.207-212
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• 1992

과잉의 CaO와 $TiO_2$를 각각 포함한 $CaTiO_3$의 결함구조를 평형상태의 전기전도도를 $85O^{\circ}C$와 $1050^{\circ}C$사이에서 산소분압의 함수로 측정하여 연구하였다. 과잉의 CaO는 A site와 B site에 나누어져서 용해되어 $Ca_{Ti}$"와 Vo", 결함을 생성하였으며, 과잉의 $TiO_2$는 $V_{Ca}$"과 Vo"을 생성했다. 평형상태의 전기전도도는 CaO 용해도 5000ppm과 $TiO_2$ 용해도 2000ppm을 각각 나타냈다. 과잉의 양이온에 의하여 생성된 산소공공은 이온전도를 하여 넓은 영역의 산소 분압에 무관한 전도도 최소값을 보였으며, 반대로 대전된 음이온 결함과 결함쌍은 관찰되지 않았다.온 결함과 결함쌍은 관찰되지 않았다.

• Journal of Mechanical Science and Technology
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• 제20권2호
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• pp.262-270
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• 2006

Direct numerical simulations (DNS) of turbulent channel flows up to $Re_{\tau}=1270$ are performed to investigate an elliptic feature and strain rate field on cross sections of coherent fine scale eddies (CFSEs) in wall turbulence. From DNS results, the CFSEs are educed and the strain rate field around the eddy is analyzed statistically. The principal strain rates (i.e. eigenvalues of the strain rate tensor) at the CFSE centers are scaled by the Kolmogorov length $\eta$ and velocity $U_k$. The most expected maximum (stretching) and minimum (compressing) eigenvalues at the CFSE centers are independent of the Reynolds number in each $y^+$ region (i. e. near-wall, logarithmic and wake regions). The elliptic feature of the CFSE is observed in the distribution of phase-averaged azimuthal velocity on a plane perpendicular to the rotating axis of the CFSE $(\omega_c)$. Except near the wall, phase-averaged maximum $(\gamma^{\ast}/\gamma_c^{\ast})$ and minimum $(\alpha^{\ast}/\alpha_c^{\ast})$ an eigenvalues show maxima on the major axis around the CFSE and minima on the minor axis near the CFSE center. This results in high energy dissipation rate around the CFSE.

• 대한화학회지
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• 제55권6호
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• pp.905-911
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• 2011

[ $C_{60}(CH_2)_nOH$ ](n=0~2)와 $C_{60}(OH)_2$의 가능한 분자구조를 B3LYP/6-311G(d,f) 이론 수준에서 최적화 하였으며, 각 화합물의 가장 안정한 분자구조(global minimum)를 확인하고 결합에너지를 계산하여 구조적 특성에 따른 에너지와의 상호연관성을 고찰하였다. 보다 정확한 상대 에너지를 계산하기 위하여 진동주파수를 계산하여 영점 진동 에너지(zero-point vibrational energy, ZPVE)를 보정하였으며, IR 스펙트럼을 예측하였다. $C_{60}(CH_2)_nOH$ (n=0-2)에서 결합에너지의 경우, $-CH_2OH$기 보다 -OH기가 결합되었을 때 결합에너지가 약 10 kcal/mol 정도 더 안정한 것으로 나타났다.

• Bulletin of the Korean Chemical Society
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• 제33권3호
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• pp.917-924
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• 2012

The conformational study of glycerol has been carried out using the M06-2X/cc-pVTZ level of theory in the gas phase and the SMD M06-2X/cc-pVTZ level of theory in water in order to understand its conformational preferences and solvation effects. Most of the preferred conformers of glycerol have two $C_5$ hydrogen bonds in the gas phase, as found by the analysis of calorimetric data. It has been known that the solvation drove the hydrogen bonds of glycerol to be weaker and its potential surface to be fatter and that glycerol exists as an ensemble of many feasible local minima in water. The calculated populations of glycerol in the gas phase and in water are consistent with the observed values, which are better than the previously calculated ones at the G2(MP2), CBS-QB3, and SM5.42 HF/6-31G(d) levels of theory.

• Journal of Astronomy and Space Sciences
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• 제32권4호
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• pp.341-348
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• 2015

New observations for the times of minimum lights of a well-known apsidal motion star CW Cephei were made using a 0.6 m wide field telescope at Jincheon station of Chungbuk National University Observatory, Korea during the 2015 observational season. We determined new times of minimum lights from these observations and analyzed O-C diagrams together with collected times of minima to study both the apsidal motion and the Light Time Effect (LTE) suggested in the system. The new periods of the apsidal motion and the LTE were calculated as 46.6 and 39.3 years, respectively, which were similar but improved accuracy than earlier ones investigated by Han et al. (2002), Erdem et al. (2004) and Wolf et al. (2006).

• 천문학회지
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• 제46권4호
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• pp.151-159
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• 2013

We discuss the orbital period changes of the Algol semi-detached eclipsing binary DI Peg by constructing the (O-C) residual diagram via using all the available precise minima times. We conclude that the period variation can be explained by a sine-like variation due to the presence of a third body orbiting the binary, together with a long-term orbital period increase (dP/dt=0.17 sec/century) that can be interpreted to be due to mass transfer from the evolved secondary component (of rate $1.52{\times}10^{-8}M_{\odot}/yr$) to the primary one. The detected low-mass third body ($M_{3min.}=0.22{\pm}0.0006M_{\odot}$) is responsible for a periodic variation of about 55 years light time effect. We have determined the orbital parameters of the third component which show a considerable eccentricity $e_3=0.77{\pm}0.07$ together with a longitude of periastron ${\omega}_3=300^{\circ}{\pm}10^{\circ}$.

• 천문학회지
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• 제47권3호
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• pp.99-104
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• 2014

We present the rst period variation study for the Algol eclipsing binary V346 Cyg by constructing the (O-C) residual diagram using all the available precise minima times. We conclude that the period variation can be explained by a sine-like variation due to the presence of a third body orbiting the binary in about $68.89{\pm}4.69$ years, together with a long-term orbital period decrease ($dP/dt=-1.23{\times}10^{-7}day/yr$) that can be interpreted to be due to slow mass loss from the ${\delta}$-Scuti primary component. The sinusoidal variation may also be explained by using the the Applegate (1992) mechanism involving cyclic magnetic activity due to star-spots on the secondary component. The present preliminary solution needs more precise photometric observations to be confirmed.