• 대한설비공학회지:설비저널
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• 제8권3호
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• pp.131-150
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• 1979

Recently only a few correlations between various factors due to the different grades of surface roughness for the nucleate pool boiling have been proposed. The main purpose of this work is to test the validity of these types of correlations between related factors to nucleate pool boiling phenomena. The boiling experiments using distilled water were carried out at the heat flux ranging from $7.4\times10^4\;to\;2.4\times10^5kcal/m^2h$ on the sintered porous metal surface with the cavity diameter of 10, n, 40, 70, $100{\mu}$, respectively, at the atmospheric pressure, To determine the bubble sizes, number of nucleation sites, delay and growth time, frequency of bubble emission and rising velocities of bubbles, the high speed motion picture technique was employed. In the correlation $f{\propto}D_b^n$, where f denotes frequency of bubble emission and $D_b$ departure diameter, n, the power factor of $D_b$, have been found to be from -2 to -10/3. The correlation C in the correlation between heat flux q and density of nucleation sites $\frac{N}{A}$, $q=C(\frac{N}{A})^n$, was appeared to be more crucial than the power factor n. The correlation of the heat flux q to the temperature difference ${\Delta}T$ and the density of nucleation sites$\frac{N}{A}$, was proposed to be $$q-460{\Delta}T^{\frac{5}{4}}=K{\Delta}T{\frac{5}{3}}(\frac{N}{A})^{\frac{2}{3}}$$. The values of heat transfer coefficient obtained in this experiments for the porous sintered metal surface appeared to be very high in comparison with the formerly obtained results for the other surfaces.

• 천문학회보
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• 제46권1호
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• pp.54.4-55
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• 2021

The Seoul National University AGN Monitoring Project (SAMP) is a welldesigned long-term AGN reverberation mapping project. SAMP focuses on the luminous AGNs out to z~0.5 with relative long time lags between AGN continuum and broad emission lines and aims to probe the high-end of the AGN broad line region (BLR) size-luminosity (R-L) relation. The pilot observations started in October 2015 for 100 AGNs to confirm the variability and the H and [O III] emission line strengths. Based on the initial variability test, 48 quasars has been continued spectroscopic monitoring since Feb. 2016 with Lick 3m and MDM 2.4m telescopes with a cadence of ~20 days. Supporting photometric monitoring in B and V band was conducted at multiple facilities including the MDM 1.3m, LOAO, and DOAO telescopes with a cadence of ~10 days. By the time of Feb. 2021, we have obtained five years spectroscopic and photometric data. More than 30 AGNs shows significant variability in five-year baseline and 16 of them show well detected lags between B-band and H. Here, we report some examples of SAMP light curves and lag detections using the first five-year data as well as the location of our 16 targets in the AGN BLR R-L relation. These measurements are consistent with the existing R-L relation and located at the high-end. With the coming data, SAMP are hopefully to report more AGNs with well detected lags. Our results demonstrate the general feasibility and potential of long-term reverberation project with medium cadence for luminous AGNs.

• 천문학회보
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• 제46권2호
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• pp.75.2-76
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• 2021

MESSIER is a science satellite project to observe the Low Surface Brightness (LSB) sky at UV and optical wavelengths. The wide-field, optical system of MESSIER is optimized minimizing optical aberrations through the use of a Linear Astigmatism Free - Three Mirror System (LAF-TMS) combined with freeform mirrors. One of the key factors in observations of the LSB is the shape and spatial variability of the Point Spread Function (PSF) produced by scatterings and diffraction effects within the optical system and beyond (baffle). To assess the various factors affecting the PSF in this design, we use PhoSim, the Photon simulator, which is a fast photon Monte Carlo code designed to include all these effects, and also atmospheric effects (for ground-based telescopes) and phenomena occurring inside of the sensor. PhoSim provides very realistic simulations results and is suitable for simulations of very weak signals. Before the application to the MESSIER optics system, PhoSim had not been validated for confocal off-axis reflective optics (LAF-TMS). As a verification study for the LAF-TMS design, we apply Phosim sequentially. First, we use a single parabolic mirror system and compare the PSF results of the central field with the results from Zemax, CODE V, and the theoretical Airy pattern. We then test a confocal off-axis Cassegrain system and check PhoSim through cross-validation with CODE V. At the same time, we describe the shapes of the freeform mirrors with XY and Zernike polynomials. Finally, we will analyze the LAF-TMS design for the MESSIER optical system.

• 천문학회보
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• 제46권1호
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• pp.41.2-41.2
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• 2021

In this study, we generate He I 1083 nm images from Solar Dynamic Observatory (SDO)/Atmospheric Imaging Assembly (AIA) images using a novel deep learning method (pix2pixHD) based on conditional Generative Adversarial Networks (cGAN). He I 1083 nm images from National Solar Observatory (NSO)/Synoptic Optical Long-term Investigations of the Sun (SOLIS) are used as target data. We make three models: single input SDO/AIA 19.3 nm image for Model I, single input 30.4 nm image for Model II, and double input (19.3 and 30.4 nm) images for Model III. We use data from 2010 October to 2015 July except for June and December for training and the remaining one for test. Major results of our study are as follows. First, the models successfully generate He I 1083 nm images with high correlations. Second, the model with two input images shows better results than those with one input image in terms of metrics such as correlation coefficient (CC) and root mean squared error (RMSE). CC and RMSE between real and AI-generated ones for the model III with 4 by 4 binnings are 0.84 and 11.80, respectively. Third, AI-generated images show well observational features such as active regions, filaments, and coronal holes. This work is meaningful in that our model can produce He I 1083 nm images with higher cadence without data gaps, which would be useful for studying the time evolution of chromosphere and coronal holes.

• 분석과학
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• 제19권1호
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• pp.65-72
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• 2006

본 연구에서는 필터를 이용하여 가스상 황화합물들을 필터 방식으로 제거하는 특성을 비교 분석하고자 하였다. 이를 위해, 이산화황으로 대표되는 산화황화합물과 황화수소를 위시한 5가지 환원황화합물 ($H_2S$, $CH_3SH$, DMS, $CS_2$, 와 DMDS)을 동시에 함유한 표준가스를 준비하였다. 그리고 이 가스를 연구대상으로 정한 글래스파이버 필터에 흘려주면서, 필터 통과 유무에 따른 농도차를 분석하였다. 이러한 자료를 토대로 황성분들의 제거특성을 각각의 황성분에 대비하여 해석하였다. 그 결과에 의하면, 이산화황은 필터에 의해 거의 완전하게 제거되지만, 환원황성분들은 각자의 반응성에 따라 상당히 차별화된 결과를 보였다. 반응성이 가장 강한 황화수소는 60% 가까이 제거되었다. 그러나 이에 반해, 분자량이 큰 성분들(DMS, $CS_2$, DMDS)은 필터에 제거되지 않고 거의 통과하는 것으로 나타났다.

• 공업화학
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• 제34권6호
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• pp.640-648
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• 2023

The purpose of this study was to determine the inhibitory effect of heavy metals [Cd(II), Ni(II), and Zn(II)] on the growth of Rhodobacter species (Rhodobacter blasticus, Rhodobacter sphaeroides, and Rhodobacter capsulatus) and their potential use for Cd(II), Ni(II), and Zn(II) bioremoval from liquid media. The presence of toxic heavy metals prolonged the lag phase in growth and reduced biomass growth for all three Rhodobacter species at concentrations of Cd, Ni, and Zn above 10 mg/L. However, all three Rhodobacter species also had a relatively high specific growth rate against each toxic heavy metal stress test for concentrations below 20 mg/L and possessed a potential bioaccumulation ability. The removal efficiency by all strains was highest for Cd(II), followed by Ni(II), and lowest for Zn(II), with the removal efficiency of Cd(II) by Rhodobacter species being 66% or more. Among the three strains, R. blasticus showed a higher removal efficiency of Cd(II) and Ni(II) than R. capsulatus and R. sphaeroides. Results also suggest that the bio-removal processes of toxic heavy metal ions by Rhodobacter species involve both bioaccumulation (intracellular uptake) and biosorption (surface binding).

• 한국해양공학회지
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• 제38권2호
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• pp.64-73
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• 2024

Oil spills pose significant threats to marine ecosystems, human health, socioeconomic aspects, and coastal communities. Accurate real-time predictions of oil slick transport along coastlines are paramount for quick preparedness and response efforts. This study used an open-source OpenOil numerical model to simulate the fate and trajectories of oil slicks released during the 2007 Hebei Spirit accident along the Korean coasts. Six combinations of input parameters, derived from a five-day met-ocean dataset incorporating various hydrodynamic, meteorological, and wave models, were investigated to determine the input variables that lead to the most reasonable results. The predictive performance of each combination was evaluated quantitatively by comparing the dimensions and matching rates between the simulated and observed oil slicks extracted from synthetic aperture radar (SAR) data on the ocean surface. The results show that the combination incorporating the Hybrid Coordinate Ocean Model (HYCOM) for hydrodynamic parameters exhibited more substantial agreement with the observed spill areas than Copernicus Marine Environment Monitoring Service (CMEMS), yielding up to 88% and 53% similarity, respectively, during a more than four-day oil transportation near Taean coasts. This study underscores the importance of integrating high-resolution met-ocean models into oil spill modeling efforts to enhance the predictive accuracy regarding oil spill dynamics and weathering processes.

• Journal of Radiation Protection and Research
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• 제41권1호
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• pp.31-39
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• 2016

연구배경: 우리나라를 포함한 중국, 대만, 북한, 일본 등에서 원전, 재처리시설과 같은 원자력시설의 증가에 따라 주변국 핵활동 분석의 종합적 대책이 필요하다. 우리나라와 포괄적핵실험금지조약기구(Comprehensive Nuclear-Test-Ban Treaty Organization, CTBTO)는 동북아시아 지역에서 핵종 탐지소를 운영 중으로, 핵종탐지 장비에서 특이 값 측정시 모니터링 자료의 분석과 더불어 배출원 탐색모델을 이용하여 핵종의 기원이 어디인지 추정하고 평가하는 것은 주변국 핵활동에 대한 감시 및 안전성 확보 측면에서 중요하다. 재료 및 방법: 주변국의 은밀한 핵활동 시 방사성핵종의 기원을 추정하기 위하여 3차원 전진/후진형 궤적모델을 개발하였다. 개발된 궤적모델은 궤적 미분방정식을 유한차분법을 이용한 방법으로 주어진 바람자료를 이용하여 방사성핵종의 방출지점으로부터 입자의 궤적을 순차적으로 찾아가는 전진형 모델과 시간 역산으로 방출기원을 추정하는 후진형 모델로 구성되었다. 결과 및 논의: 개발된 궤적모델의 검증을 위하여 체르노빌 사고 당시 측정된 농도자료를 이용하였다. 검증결과 관측지점의 농도가 높게 측정된 지점과 방출기원에서 가까운 지역으로부터 시간 역산의 방출지점을 추정한 결과의 정확도가 높았다. 3차원 궤적모델은 방출시간, 방출높이, 방출간격 등의 변수에 의해 계산결과가 달라지는 불확도를 내포하고 있는데, 이러한 궤적모델의 불확도를 최소화하기 위해 한국원자력연구원에서 개발한 대기확산모델(long-range accident dose assessment system, LADAS)를 이용하여 fields of regards (FOR) 기법에 의해 오염물 방출영역을 추정한바 신뢰성 있는 결과를 얻었다. 결론: 본 연구를 통하여 개발된 배출원 탐색모델은 주변국의 은밀한 핵활동 시 핵종 탐지장비와 연계하여 방사성핵종의 방출지역과 기원을 파악하여 우리나라의 핵종탐지 능력을 향상하고 핵활동 및 방사선 안전 분야에서 주도적 역할을 할 수 있을 것으로 생각된다.

• 한국대기환경학회지
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• 제32권5호
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• pp.501-512
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• 2016

The study evaluated methods to measure condensable fine particles in flue gases and measured particulate matter by fuel and material to get precise concentrations and quantities. As a result of the method evaluation, it is required to improve test methods for measuring Condensable Particulate Matter (CPM) emitted after the conventional Filterable Particulate Matter (FPM) measurement process. Relative Standard Deviation (RSD) based on the evaluated analysis process showed that RSD percentages of FPM and CPM were around 27.0~139.5%. As errors in the process of CPM measurement and analysis can be caused while separating and dehydrating organic and inorganic materials from condensed liquid samples, transporting samples, and titrating ammonium hydroxide in the sample, it is required to comply with the exact test procedures. As for characteristics of FPM and CPM concentrations, CPM had about 1.6~63 times higher concentrations than FPM, and CPM caused huge increase in PM mass concentrations. Also, emission concentrations and quantities varied according to the characteristics of each fuel, the size of emitting facilities, operational conditions of emitters, etc. PM in the flue gases mostly consisted of CPM (61~99%), and the result of organic/inorganic component analysis revealed that organic dusts accounted for 30~88%. High-efficiency prevention facilities also had high concentrations of CPM due to large amounts of $NO_x$, and the more fuels, the more inorganic dusts. As a result of comparison between emission coefficients by fuel and the EPA AP-42, FPM had lower result values compared to that in the US materials, and CPM had higher values than FPM. For the emission coefficients of the total PM (FPM+CPM) by industry, that of thermal power stations (bituminous coal) was 71.64 g/ton, and cement manufacturing facility (blended fuels) 18.90 g/ton. In order to estimate emission quantities and coefficients proper to the circumstances of air pollutant-emitting facilities in Korea, measurement data need to be calculated in stages by facility condition according to the CPM measurement method in the study. About 80% of PM in flue gases are CPM, and a half of which are organic dusts that are mostly unknown yet. For effective management and control of PM in flue gases, it is necessary to identify the current conditions through quantitative and qualitative analysis of harmful organic substances, and have more interest in and conduct studies on unknown materials' measurements and behaviors.

• 자원환경지질
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• 제55권4호
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• pp.407-419
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• 2022

메탄(CH₄)이 유출되는 관정 주변에서 토양(비포화대) 가스 모니터링과 자료 해석 방법을 제시하고자 토양 가스의 성분변화를 약 3일간 측정하였다. 이를 위해서 포항 지역의 시험 관정 2개(TB2, TB3)의 주변 1 m 이내에서 방사상으로 토양 가스를 채취하고 현장에서 CO₂, CH₄, N₂, O₂의 농도를 분석하였다. TB2의 관정 정두(wellhead)에서 30 cm 떨어진 지점에서 CO₂ 플럭스도 측정하였다. 아울러 TB2 관정 정두의 가스 시료와 대기 시료도 채취하여 분석하였다. 모니터링 마지막 날 채취한 시료는 실험실에서 CO₂의 탄소동위원소(δ¹³C_CO2)를 분석하였다. 서로 12.7 m 떨어져 있는 두 시험 관정 중 TB3는 시멘팅이 되어 있고, TB2는 시멘팅이 되어 있지 않았다. 생지구화학 반응 기반(process-based) 해석을 적용한 결과, 비포화대 가스의 CO₂, O₂, N₂ 농도와 N₂/O₂ 의 변화는 모두 CH₄의 산화를 지시하는 선과 가스의 용해에 의한 농도의 변화를 지시하는 선 사이에 위치하고 있었다. 또한 TB2 정두에서 측정된 CH₄은 대기의 CH₄에 비해서 5.2배 높은 값을 나타나고 있었다. 시멘팅이 되어 있지 않은 관정(TB2) 주변 비포화대에서 나타난 높은 CO₂ 농도(평균 1.148%)는 CH₄의 산화에 의해 증가한 것으로 판단된다. 반면, 시멘팅이 된 관정(TB3) 주변의 비포화대 CO₂는 상대적으로 낮은 농도(0.136%)를 나타내고 있었다. 따라서 CH₄가 산출되는 관정의 주변 토양가스(CO₂ 포함)는 관정의 완결 상태(시멘팅)에 크게 영향을 받는 것으로 판단된다. 본 연구는 천연가스 개발 관정 주변 토양의 환경 모니터링을 위한 전략 수립에 활용될 수 있으며, CO₂ 지중저장을 위한 주입정 및 관측정 주변 누출 감시에 활용될 수 있다. 또한 본 연구의 방법은 천연가스 저장소, 유류 오염 토양의 모니터링에 활용 가치가 있다.