• 생태와환경
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• 제39권1호통권115호
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• pp.100-109
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• 2006

본 연구는 영양염이 풍부한 하수처리수를 이용한 인공수로에서 사상성 부착조류의 성장에 미치는 요인들(유속. 부착기질, 인 농도)을 평가하였다. 실험은 하수처리수를 이용한 현장 인공수로와 실내 순환수로에서 부착조류의 성장실험을 수행하였고, 서로 다른 인 농도에서의 사상성 부착조류 종간의 성장률과 인 흡수율을 비교하였다. 조절된 유속조건(5 ${\sim}$ 15 cm $s^{-1}$)에서 사상성 부착조류의 순생산성은 유속이 빠를수록 높았으나 최대의 순생산성은 10 cm $s^{-1}$ 유속에서 나타났다. 현장 인공수로와 실내순환수로 실험 간에 사상성부착조류의 최대성장은 기질에 따라 다르게 나타났다. 부유물질이 충분히 제거되지 않았던 현장 인공수로 실험에서는 망목이 20 mm인 철망에서, 실내순환수로 실험에서 사상성 부착조류의 성장은 자연섬유망에서 높게 나타났다. 0.05 ${\sim}$ l.0 mg P $L^{-1}$로 조절된 인 농도범위에서 3종의 사상성 부착조류 성장률은 인 농도가 높아짐에 따라 증가하였으나, 각 종들은 인 농도에서 따라 차별적인 성장을 나타냈다. 또한 영양염 농도가 매우 높은 환경에서 사상성 부착조류 생물량의 발달이 크면 클수록 높은 유속이 사상체의 탈리를 유발하여 조류의 성장을 감소시키는 제한요인으로 작용할 수 있음이 제시되었다. 탈리된 사상체는 연결된 하천, 저수지, 하류의 수질과 생태계를 악화시킬 수 있기 때문에 하천 수질관리에 있어 중요한 요인으로 고려한 필요성이 크다.

• International Journal of Aeronautical and Space Sciences
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• 제2권1호
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• pp.12-19
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• 2001

Study of turbulent mixing layers has been a popular subject from the point of view of both practical application and phenomenological importance in engineering field. Turbulent mixing layers can be applied in many fields where rapid transition to turbulence is desirable in order to prevent boundary layer separation or to enhance mixing. The ability to control mixing, structure and growth of the shear flow would obviously have a considerable impact on many engineering applications. In addition to practical applications, free shear flows are one of the simplest flows to understand the fundamental mechanism in the transition process to turbulence. After the discovery of large-scale vortical structure in free shear flows many researchers have investigated the physical mechanism of generation and dissipation processes of the vortical structure. This study investigated the role of the large-scale vortical structures in the turbulent mixing layer using LES(Large-Eddy Simulation). The result shows that the pairing interaction of the vortical structure plays an important role in the growth rate of a mixing layer. It is found that the turbulence quantities depend strongly on the velocity ratio. It is also found that the vorticity in the high-velocity-side can extract energy from the mean flow, while the vorticity in the low-velocity-side lose energy by the viscous dissipation. Finally the results suggest the guideline to obtain the desired flow by control of the velocity ratio.

• 한국결정성장학회지
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• 제18권3호
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• pp.122-124
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• 2008

The partial phase diagram of $NaNO_3$-NaCl system was investigated and the eutectic temperature was determined as $294.5^{\circ}C$. A typical rod eutectics of $NaNO_3$-4.56 wt%NaCl was directionally solidified. The results of interrod spacing, ${\lambda}_E$ as a function of growth velocity, V, were. obtained as ${\lambda}_E\;V^{0.39}\;=\;5.26$ (temperature gradient, $G_l\;=\;21.4^{\circ}C/mm$) and ${\lambda}_E\;V^{0.32}\;=\;5.45$ ($G_l\;=\;3.9^{\circ}C/mm$) and the exponent numbers of growth velocity were smaller than the theoretical value, 1/2. The sample rotation applied during directional solidification made the interrod spacing decrease slightly.

• 한국주조공학회지
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• 제17권4호
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• pp.379-384
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• 1997

Al-15Cu-lMg alloys have been directionally solidified in 3mm diameter alumina tubes under the conditions of $760^{\circ}C$ of furnace temperature and 12 cm/hr of furnace moving velocity(V). By analyzing the evolution of the temperature profiles along the alloy length, the position of the solid/liquid interface, temperature gradient(G) and local growth velocity (R) were determined. These growth characteristics were compared for 6, 10, 14 cm length alloys. Steady state growth region was obtained in 15 cm length alloy, not in 6, 10 cm.

• 천문학회보
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• 제36권1호
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• pp.52.2-52.2
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• 2011

The correlation between black hole mass and galaxy stellar velocity dispersion gives an important clue on the black hole growth and galaxy evolution. In the case of AGN, however, it is extremely difficult to measure stellar velocity dispersions in the optical spectra since AGN continuum dilutes stellar absorption features. In contrast, stellar velocity dispersions of active galaxies can be measured in the near-IR, where AGN-to-star flux ratio is much smaller, particularly with the laser-guide-star adaptive optics. However, it is crucial to test whether the stellar velocity dispersion measured from the near-IR spectra is consistent with that measured from the optical spectra. Using the TripleSpec at the Palomar 5-m Telescope, we obtained high quality spectra ranging from 1 to 2.4 micron for a sample of 35 nearby galaxies, for which dynamical black hole masses and optical stellar velocity dispersion measurements are available, in order to calibrate the stellar velocity dispersion in the near-IR. In this poster, we present the initial results based on 10 galaxies, with the stellar velocity dispersion measured in the H-band.

• 대한기계학회논문집B
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• 제20권10호
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• pp.3322-3333
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• 1996

A numerical analysis has been conducted to investigate a modified floating-zone crystal growth process in which most of the melt surface is covered with a heated ring. The crystal rod is not only pulled downward but rotated around its axisymmetric line during crystal growth process in order to produce the flat interface of crystal growth and the single crystal growth of NaNO3 is considered in 6mm diameter. The present study is made from a full-equation-based analysis considering a pulling velocity in all of solid and liquid domains and both of solid-liquid interfaces are tracked simultaneously with a governing equation in each domain. Numerical results are mainly presented for the comparison of the surface shape of rotational crystal rod with that of no-rotational crystal rod and the effects of revolution speeds of the crystal rod. Results show that the rotation of crystal rod produces more its flat surface. In addition, the shape of crystal growth near the centerline is more concaved with the increase in the revolution speed of crystal rod. The flow pattern and temperature distribution is analyzed and presented in each case. As the pulling velocity of crystal rod is increasing, the free surface of the melt below the heated ring is enlarged due to the crystal interface migrating downward.

• 대한기계학회논문집
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• 제16권8호
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• pp.1519-1529
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• 1992

본 연구에서는 단열 전단 밴드의 특성 규명을 위하여 특별히 고안된 계단 형 상 시편(stepped specimen)의 수치해석을 통하여 단열 전단 밴드의 형성과 성장(init- iation and growth of adiabatic shear band)에 관한 체계적 해석을 시도해 보았다. 금번 논문에서는 우선 격자 크기(mesh size)와 충격 속도(impact velocity)가 단열 전 단 밴드의 형성 및 성장에 미치는 영향과 제반 특성을 규명할 계획이며 차후 재료의 기하학적 형상 등이 단열 전단 밴드의 형성 및 성장에 미치는 영향에 대해서도 단계적 연구를 시도할 계획이다. 해석을 위하여 가공경화효과, 변형률 속도 경화효과(stra- in rate hardening effect), 열적연화효과 등을 고려할 수 있는 구성 방정식(constit- utive equation)을 갖춘 엑스플리시트 시간적분 유한요소 코드(explicit time integr- ation finite element code)를 사용하였으며 기존의 연구 결과와는 달리 어떠한 인위 적 결함도 해석에 사용하지 않았다.

• 보건교육건강증진학회지
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• 제6권1호
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• pp.75-90
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• 1989

This study tries to show the physical growth patterns and various adolescent characteristics by using longitudinal data for the height, weight, chest girth and sitting height of 1, 132 high school students in Seoul. And this study also tries to show what influencing factors on the physical growth of this aged population. The followings are the results. 1. The boys have their peak velocity of height when they are 12~13 years old. And the girls have when they are 10~11 years old. Peak velocity of weight for boys is at the age of 13~14. And for girls is at the age ofr11~12. Peak velocity of chest girth for boys is at the age of 12~13. And for girls is at the age of 11~12. Peak velocity of sitting height for boys is at the age of 13~14. And for girls is at the age of 11~13. So girls of this period grow more rapidly by around two years than boys. 2. The menarche of girls begins at the age of 12.4. So it begins 1.4 year before peak height velocity period. 3. Of life behavior boys contingency coefficient between essential time and height and weight is .5150 and .479 5, that between studying time and height and weight is .3344 and and .2912(In case of girls is .4735, .4321, .3247, .3134).

• 한국해양공학회지
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• 제12권2호통권28호
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• pp.111-120
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• 1998

Laboratory settling experiments (column, recirculating flume) were conducted for further understanding of the physical processes of cohesive sediment transport. \In still water experiments, the growth rate of flocculation is dependent upon the initial suspended concentration. Consequently, the settling velocity increases with concentration of flees. In flocculation settling regime, the exponent n in the settling velocity, $w_s=kC^n$, for Nakdong estuary mud was obtained empirically. The exponents were found to be 1.33, and 1.06 for the initial suspended concentrations of 1 g/i and 3 g/t, respectively. In flowing water, experiments for the median settling velocity with Nakdong mud in a recirculating flume were conducted. Settling velocity was found to depend much more strongly on the current velocity than initial concentrations. The temporal variation of suspended concentration increases as current velocity decreases.

• 한국결정학회지
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• 제5권2호
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• pp.93-99
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• 1994

K2O/3MOOS/0.SBB03 융제를 사용하여 TSSG 법으로 육성한 Md:Yal3(BO3)4 (NYAB) 단결정의 결정외형 및 표면형상을 연구하였다. <100>과 <120> 종자정을 사용한 경우는 서로 다른 크기의 프리즘 면들과 (101) 면들이 발달하였고 <001> 종자정을 사용하였을 때는 (001) 면이 함께 발달하였다. 종자정의 방향이 <100>또는 <120> 일때 프리즘 면 위에 성장구룽이 많이 형성되었으나, <001> 일때는 이웃하는 (101) 면에 평행한 줄무늬가 형성 되었다. (101) 면은 이차원 핵생성에 의한 성장이 지배적이고, <001> 종지정을 사용할 때 발달하는 (001) 면은 나선형 전위에 의한 성장이 지배적이었다. 종자정의 방향은 성장외형을 변화시키고 성장외형과 결정의 질을 결정하는 중요한 성장변수로 작용하였다.