• Journal of Wetlands Research
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• v.8 no.3
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• pp.91-103
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• 2006

The objective of this study is to analyze the characteristics of flow and bed change at the wide, shallow confluence of the Geum river and Mihocheon, which has different bed slope, height, and sediment concentration condition between the main channel and tributary. RMA-2 and SED2D were used to simulate flow and bed changes at the site. Flow simulations showed that the overall flow velocity, shear layer and vortex generated at the left bank of the confluence increase as the discharge was increased. Sediment transport simulations indicated that because of the high inflow sediment concentration from Mihocheon, sediment concentration in the main river increases after the confluence, the high sediment concentration band was kept along the shear layer boundary and the left bed was aggraded after confluence.

• Publications of The Korean Astronomical Society
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• v.27 no.4
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• pp.281-284
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• 2012

We utilize AKARI's slitless spectroscopic capability to detect the $3.3{\mu}m$ polycyclic aromatic hydrocarbons (PAHs) emission and measure star formation (SF) activity for various AKARI programs. First, we obtain $2{\sim}5{\mu}m$ spectra of 20 flux-limited galaxies with mixed SED classes in order to calibrate the $3.3{\mu}m$ PAH luminosity ($L_{PAH3.3}$) as a star formation rate (SFR) indicator. We find that $L_{PAH3.3}$ correlates with $L_{IR}$ as well as with the $6.2{\mu}m$ PAH luminosity ($L_{PAH6.2}$). The correlations does not depend on SED classes. We find that ULIRGs deviate from the correlation between PAH luminosities and $L_{IR}$, while they do not for the correlation between PAH luminosities. We suggest possible effects to cause this deviation. On the other hand, how AGN activity is linked to SB activity is one of the most intriguing questions. While it is suggested that AGN luminosity of quasars correlates with starburst (SB) luminosity, it is still unclear how AGN activity is connected to SF activity based on host galaxy properties. We are measuring SFRs for the LQSONG sample consisting of reverberation mapped AGNs and PG-QSOs. This is an extension of the ASCSG program by which we investigated the connection between SB and AGN activities for Seyferts type 1s at z ~ 0.36. While we found no strong correlation between $L_{PAH3.3}$ and AGN luminosity for these Seyferts 1s, $L_{PAH3.3}$ measured from the central part of galaxies correlates with AGN luminosity, implying that SB and AGN activities are directly connected in the nuclear region.

• Proceedings of the Korea Water Resources Association Conference
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• 2008.05a
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• pp.963-966
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• 2008

본 연구에서는 최근까지 유사관측을 수행하고 있는 금강본류 하도구간의 금남$\sim$공주 지점을 대상으로 하였다. 분석을 위하여 이 지점의 총유사량 산정에 영향을 미치는 부유사량 관측 및 수위, 유량과 같은 하천 흐름 등에 관한 과거의 자료를 수집 정리 하였다. 본 연구에서 적용하고자 하는 교량의 교각에 대한 기하학적 형상은 원형, 정사각형, 정팔각형, 장방형으로 하였으며 분석 모형은 SED2D-WES 모형을 이용하여 유역에 대한 교각의 형상이 미치는 영향에 대하여 연구 하였다. 그 결과 지름이 6m, 경간장 57m인 원형교각의 경우 교각에서 약 14.3m 떨어진 곳에서 최고 유속 0.75m/s가 발생되었으며, $6{\sim}6m$의 정사각형교각의 경우 교각으로부터 약 15.8m떨어진 곳에서 0.68m/s의 최대 유속이 발생하고 $6{\sim}6m$ 정팔각형교각의 경우 교각으로부터 약 16.2m떨어진 곳에서 0.65m/s의 최대유속이 발생하고, 마지막으로 $3{\sim}6m$ 장방형교각의 경우 교각으로부터 약 21m 떨어진 구간에서 0.63m/s의 최고 유속이 발생하는 것으로 나타났다. 대상유역의 길이가 길고, 유속이 낮으므로 유출지점까지 흘러내려가는 유사량보다 하천내에 유입된 유사가 그대로 퇴적되는 경우가 많아 24시간 분석결과 하상변동량은 퇴적량과 침식량을 합하여 약 0.22%정도 변동되는 것으로 나타났으며, 교각형상에 따른 하상변동특성으로 원형교각의 경우 세굴이 일어나는 지점은 교각에서 약 16.88m떨어진 지점까지 하상변동이 일어났으며, 정사각형 교각의 경우 교각에서 약 10.96m떨어진 지점까지, 정팔각형 교각의 경우 교각에서 약 6.32m떨어진 지점까지, 장방형 교각의 경우 교각에서 약 18.23m떨어진 지점까지 하상변동이 나타남을 알 수 있었다.

• Radiation Oncology Journal
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• v.6 no.2
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• pp.151-154
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• 1988

To answer the question whether last clonogenic cell should be eradicated for the tumor to be controlled, radiation tumor control study was performed using microscopic tumors of variable sizes ranging from 101 to 10s tumor cells. $TCD_{50}'s$ estimated from experimental data were 14.8, 27. 1, 42.4, 49.9 and 65.5 Gy for $10^1,\;10^2,\;10^3,\;10^4\;and\;10^4$ tumor cells, respectively. Theoretical calculations, assuming that all the clonogenic cells should be inactivated, were 15.65, 8.50, 40.97, 53.41 and 65.85 Gy. From this well matched data, it can be concluded that all the clonogenic cells should be eradicated for tumor control, at least in this tumor model.

• Journal of Korea Water Resources Association
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• v.42 no.4
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• pp.319-329
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• 2009

Sediment release openings or pipes are installed in the flood control dam constructed to reduce flood damages, which are to allow water and sediments pass through the dam and to prevent flow blockage and sedimentation in the upstream area of the dam. The Hantan River Flood Control Dam (HRFCD) has been projected for flood damage reduction and sediment release openings and ecological passages are considered for the dam design. In this study, sediment deposition due to the construction of HRFCD was analyzed using the HEC-6 model and compared with the state before the dam construction with respect to the conditions of the annual mean daily discharge and annual discharge hydrograph. According to the numerical results, although downstream water levels were changed by the dam structure, the effects of bed changes were not propagated from the dam over 2 km upstream. Also, 2D numerical models of RMA2 and SED2D were used to predict bed changes in the upstream area with and without sediment release openings. Consequently, it is presented that sediment release openings decreased maximum deposition height in the upstream channel of the dam.

• Journal of Korean Vacuum Science & Technology
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• v.6 no.1
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• pp.8-11
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• 2002

Ni, Si and $SiO_2$ films were implanted by 350 keV B $i_{+}$ ions at room temperature with fluences of 1$\times$10$^{16}$ and 2$\times$10$^{16}$ ions/c $m^2$ The depth distributions of implanted B $i^{+}$ ions in Ni, Si and $SiO_2$ films were by investigated by Rutherford backscattering. The results show that the depth distributions of implanted B $i^{+}$ ions into Ni, Si and $SiO_2$ films have obeyed nearly Gaussian distributions. The maximum difference between experimental and calculated values is less than 18 % for mean projected range. Experimental range straggling deviated significantly from calculated value. The possible reasons are discussed.sed.d.

• The Bulletin of The Korean Astronomical Society
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• v.40 no.1
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• pp.52.2-52.2
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• 2015

In astronomical observations, stable auto-guiding and accurate target centering capabilities are critical to increase observation efficiency and sensitivity. Recently, Center for the Exploration of the Origin of the Universe (CEOU) has developed SQUEAN (SED camera for QUasars in EArly uNiverse). SQUEAN is installed and had successful observations at the 82 inch Otto Struve Telescope of McDonald Observatory in 2015 February. We have upgraded the existing auto-guiding softwares to KAP82 (KHU Auto-guiding Package for the McDonald 82 inch Telescope). Keeping the original hardware systems and the software algorithms of CAP (CQUEAN Auto-guiding Package), KAP 82 is completely re-written in Visual C++. We developed several center finding algorithms, e.g., 2D-gaussian fitting and weighted mean methods. In this presentation, we compare the auto-guiding performances with these algorithms.

• Proceedings of the Korea Water Resources Association Conference
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• 2005.05b
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• pp.1154-1158
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• 2005

본 연구에서는 2002년 여름 전국을 강타한 태풍 '루사'에 의한 집중호우와 관련하여 충북 영동군 일원에 발생한 하천범람에 따른 침수피해에 대해 하천의 수위 상승과 하천변 제내지의 침수에 따른 수리특성을 분석하였다. 이를 위해 홍수유출량 산정에 HEC-HMS모형과 HEC-GeoHMS모형을 사용하였고, 외수위 변동을 해석하기 위해서 HEC-RAS를 이용하여 부정류 해석을 수행하였다. 또한 침수구역의 수리특성과 하상변동, 유사분포 모의를 위해 RMA2, SED2D 모형을 적용하였다. 그 결과 하천범람시 유속은 $2.6m/sec\~3.4m/sec$ 분포를 나타내었고, 하상변동의 경우 제방에 근접한 곳에서 제방 절개부와 가까운 지역은 $0.15m\~0.17m$정도 유사가 퇴적되는 것으로 분석되었다.

• Proceedings of the Korea Water Resources Association Conference
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• 2011.05a
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• pp.344-348
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• 2011

본 연구에서의 낙동강 본류에 설치예정인 N보를 중심으로 수문조건에 따른 흐름특성을 연구하기 위하여 N수위표에서 상류방향으로 약 4km구간을 채택하였다. 분석에서는 수위표 상류 약2.5km지점에 보를 설치하여 수문의 개방도와 수문조건에 따라 보의 상 하류 구간의 수리학적 특성 및 하상변화의 분석을 실시하였다. 그 결과 유속 수심 및 하상변동은 보에서 배수되는 유량과 밀접한 관계가 있다고 판단되며 차후 유황에 따른 수문의 개방도를 적절히 계획 설계하여 보다 안정적인 치수계획을 수립해야 할 것으로 판단된다.

• The Bulletin of The Korean Astronomical Society
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• v.43 no.2
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• pp.52.2-52.2
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• 2018

The shape of a galaxy's spectral energy distribution ranging from ultraviolet (UV) to infrared (IR) wavelengths provides crucial information about the underlying stellar populations, metal contents, and star-formation history. Therefore, analysis of the SED is the main means through which astronomers study distant galaxies. However, interstellar dust absorbs and scatters UV and optical light, re-emitting the absorbed energy in the mid-IR and Far-IR. I present the updated 3D Monte-Carlo radaitive transfer code MoCafe to compute the radiative transfer of stellar, dust emission through a dusty medium. The code calculates the emission expected from dust not only in pure thermal equilibrium state but also in non-thermal equilibrium state. The stochastic heating of very small dust grains and/or PAHs is calculated by solving the transition probability matrix equation between different vibrational, internal energy states. The calculation of stochastic heating is computationally expensive. A pilot study of radiative transfer models of SEDs in clumpy (turbulent), galactic environments, which has been successfully used to understand the Calzetti attenuation curves in Seon & Draine (2016), is also presented.