• 한국군사과학기술학회지
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• 제17권1호
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• pp.122-128
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• 2014

Remote fourier transform infrared(FTIR) chemical imaging detection system allows detection and identification of gases in the atmosphere from long distances. In this paper, the appropriate field of view(FOV) of the FTIR imaging system was examined and the main performance of the system for the interferometer was described. For the determination of the FOV, simulations of gas dispersion range were performed with the NBC reporting and modeling software(NBC-RAMS) developed by ADD. As a result, minimum 192 mrad of FOV was required for the remote FTIR imaging system to visualize chemical warfare agents dispersed in several hundred meters. At the same time, 0.75 mrad of instantaneous field of view(IFOV) for a linear interferometer proper to take a FOV for the chemical agent imaging.

• Nuclear Engineering and Technology
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• 제51권3호
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• pp.792-799
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• 2019

The present study aims to investigate the fluorination of thorium oxide ($ThO_2$) by ammonium hydrogen difluoride ($NH_4HF_2$). Fluorination was performed at room temperature by mixing $ThO_2$ and $NH_4HF_2$ at different molar ratios, which was then left to react for 20 days. Next, the mixtures were analyzed using X-ray diffraction (XRD) at the intervals of 5, 10, 15, and 20 days, followed by the heating of the mixtures at $450-750^{\circ}C$ with argon gas flow. The characterization of $ThF_4$ was established using X-ray diffraction (XRD) and scanning electron microscopy-dispersion X-ray spectroscopy (SEM-EDX). In this study, ammonium thorium fluoride was synthesized through the fluorination of $ThO_2$ at room temperature. The optimum molar ratio in synthesizing ammonium thorium fluoride was 1.0:5.5 ($ThO_2:NH_4HF_2$) with 5 days reaction time. In addition, the heating of ammonium thorium fluoride at $450^{\circ}C$ was sufficient to produce $ThF_4$. Overall, this study proved that $NH_4HF_2$ is one of the fluorination agents that is capable of synthesizing $ThF_4$.

• 천문학회보
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• 제43권2호
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• pp.35.2-35.2
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• 2018

Using the K-band Multi-object Spectrograph (KMOS) at the Very Large Telescope (VLT), the KMOS Redshift One Spectroscopic Survey (KROSS) has gathered integral-field data for ~800 star-forming galaxies at a redshift z~1, when the universe was roughly half its current age and forming the bulk of its stars. With spatially-resolved observations, KROSS reveals galaxies that are both gas-rich and highly turbulent. It is possible to derive the observed and baryonic Tully-Fisher (luminosity - rotation velocity) relations, thus constraining the mass-to-light ratios and total (luminous + dark) masses of the galaxies. This in turn highlights the dependence of the relation zero-point on the degree of rotational support of the galaxies (rotational velocity to velocity dispersion ratio). By degrading and analogously analysing integral-field data of hundreds of local galaxies from the Sydney-AAO Multi-object Integral-field Spectrograph (SAMI) survey, a robust comparison z=0 Tully-Fisher relation can also be derived, thus further constraining the luminous and dark mass growth of disk galaxies over the last 7 billions years. This unique comparison also reveals that systematic effects associated with sample selection and analysis methods are as large as the effects expected from cosmological evolution, and thus that most other comparisons employing heterogeneous data and/or methods can safely be ignored.

• 한국초전도ㆍ저온공학회논문지
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• 제10권1호
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• pp.1-5
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• 2008

The effect of $BaCeO_3$ doping on the critical current density of YBCO film by TFA-MOD method was studied. $BaCeO_3$ doping was made by two method; one is direct addition of $BaCeO_3$ nano-sized powder prepared by citrate process followed by grinding with planetary ball mill for 10 hours. Another is addition of Ba-Ce precursor solution prepared with Ba-acetate and Ce acetate dissolved in TFA to the YBCO-TFA precursor solution. The film was made by standard dip coating and heat treatment process with conversion temperature of $790^{\circ}C$ in 1000 ppm oxygen containing moisturized Ar gas atmosphere. The direct addition of $BaCeO_3$ powder resulted in YBCO film with good epitaxial growth and no evidence of second phase formation. The addition through precursor solution resulted in the increase of critical current density upto 30 at% doping and uniform dispersion of $BaCeO_3$ fine inclusion was confirmed by SEM-EDX.

• 천문학회보
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• 제46권2호
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• pp.68.3-69
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• 2021

We present a novel profile stacking technique based on optimal profile decomposition of a 3D spectral line data cube, and its performance test using the HI data cubes of sample galaxies from HI galaxy surveys, THINGS and LITTLE THINGS. Compared to the previous approach which aligns all the spectra of a cube using their central velocities derived from either moment analysis, single Gaussian or hermite h3 polynomial fitting, the new method makes a profile decomposition of the profiles from which an optimal number of single Gaussian components is derived for each profile. The so-called superprofile which is derived by co-adding all the aligned profiles from which the other Gaussian models are subtracted is found to have weaker wings compared to the ones constructed in a typical manner. This could be due to the reduced number of asymmetric profiles in the new method. A practical test made on the HI data cubes of the THINGS and LITTLE THINGS galaxies shows that our new method can extract more mass of kinematically cold HI components in the galaxies than the previous results. Additionally, we fit a double Gaussian model to the superprofiles whose S/N is boosted, and quantify not only their profile shapes but derive the ratio of the Gaussian model parameters, such as the intensity ratio and velocity dispersion ratio of the narrower and broader Gaussian components. We discuss how the superprofile properties of the sample galaxies are correlated with their other physical properties, including star formation rate, stellar mass, metallicity, and gas mass.

• 한국진공학회지
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• 제18권1호
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• pp.1-8
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• 2009

고분자 Polystyrene (PS)의 표면에 친수성을 가지게 하기 위하여 RF power를 150 W에서 350 W로 처리 시간을 1회에서 4회로 처리하며, 압축된 공기와 산소 가스를 사용하여 상압 플라즈마로 개질하였다 압축된 공기로 처리한 시료의 접촉각은 $91^{\circ}$에서 $20^{\circ}$까지 접촉각이 낮아졌으며, 이 때 표면 에너지는 45.74에서 68.48 dyne/cm 증가하였다. 동일한 조건에서 산소 가스로 300 W의 RF Power로 4회 처리하였을 때 접촉각이 $91^{\circ}$에서 $17^{\circ}$로 변화하였으며, 표면에너지는 45.74에서 69.73 dyne/cm 증가하였다. 표면에너지의 증가는 dispersion force의 증가보다는 polar force의 증가에 의한 것으로 보인다. 상압 플라즈마로 처리된 시료의 접촉각 감소와 표면에너지의 증가는 X-ray photoelectron spectroscopy (XPS)의 spectra 결과로부터 PS의 표면에 C-O, C=O 결합의 증가로 인한 친수성 작용기가 표면에 형성되었기 때문이라고 생각된다. 상압 플라즈마 처리 후 대기 중에 보관된 시료의 접촉각은 시간이 경과함에 따라 증가하지만 물 속에 보관된 시료의 경우는 상압 플라즈마 처리 후의 접촉각을 그대로 유지하였다. 상압 플라즈마를 이용하여 PS의 표면을 개질하고, 그 위에 $4,000\;{\AA}$과 $8,000\;{\AA}$의 구리 박막을 열증착법을 이용하여 증착하였다. 각 시료와 구리 박막의 계면과의 접착력은 테이프 테스트 (ASTM D3359)를 이용하여 처리된 PS 표면이 처리하지 않은 시편에 비하여 접착력이 향상되었음을 확인하였다.

• 한국지하수토양환경학회:학술대회논문집
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• 한국지하수토양환경학회 2001년도 총회 및 춘계학술발표회
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• pp.98-103
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• 2001

부산 석대 생활폐기물 매립지의 환경오염 특성을 파악하기 위해 매립장 지역의 가스발생량 측정, 침출수 및 토양시료 채취, 지구통계학적, 수리지질학적 및 지구화학적 분석과 실내 주상시험을 실시하여, 침출수의 오염 부하량과 가스발생량, 가스의 농도와 지반 침하, 지질매체의 특성, 침출수의 오염 부하량과 가스발생량, 가스의 농도와 지반 침하, 지질매체의 특성, 침출수의 이동 및 확산의 관계를 고찰하였다. 그리고 물수지분석을 통하여 침출수의 발생량과 오염 부하량을 선정하였다. 매립장 A지구로부터 36개 가스정에서 획득한 가스자료를 $O_2$C $H_4$ $H_2$S, CO의 4가지 성분에 대해 지구통계학적 기법으로 분석한 결과, 다른 지점에 비해 가스의 농도가 높은 지점 주변에서 부분적으로 지반 침하가 발생하는 것으로 나타났다. Leachate-1, 2, 3에서 채취한 침출수의 화학적 분석 결과, 전기전도도와 Total Alkalinity는 높게 나타났으나, Cl, Cr, Mn, Cu, Zn, Cd, Pb 등이 과거보다 감소하였고, 수질유형은 삼각다이아그램에서 Na-HC $O_3$형으로 나타난다. Leachate-1, 2, 3에서 채취한 침출수의 화학적 분석 결과 전기전도도와 Total Alkalinity는 다이아그램에서 Na-HC $O_3$형으로 나타난다. 수질분석 결과에 의하면 생활폐기물의 생분해가 아직도 계속해서 활발히 진행되고 있는 것으로 판단된다. 물수지분석 결과, 순수하게 지하로 침투하는 침출수량은 약 465.11㎥/day이고, Cl, Mn, Fe의 순수오염 부하량은 각각 223.8kg/day, 0.2kg/day, 0.3kg/day로 추정된다. 매질에 대한 실내 주상시험에서 기반암 풍화토와 매립토에 대한 선형유속(equation omitted)은 각각 0.206cm, 0.019cm, 확산계수( $D_{ι}$)는 각각 0.234$\textrm{cm}^2$/min, 0.118$\textrm{cm}^2$/min, 종분산 지수 ($\alpha$$_{ι}$)는 각각 1.136cm, 0.095cm로 복토재로 사용된 매립토보다 기반암풍화토가 오염물질의 확산속도가 더 큰 것으로 나타났다.

• 공업화학
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• 제18권3호
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• pp.245-250
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• 2007

실리카겔의 열처리 온도에 따른 1,2-dichlorobenzene의 흡착 특성을 모멘트 법으로 고찰하였다. 실리카겔의 열처리 온도는 150, 500, $800^{\circ}C$로 변화시켰으며 고정층 반응기를 사용하여 TCD (Thermal Conductivity Detector)가 장착된 기체크로마토 그래프에서 1,2-dichlorobenzene의 펄스 응답곡선을 측정하였다. 1,2-dichlorobenzene의 평형흡착상수와 표면 흡착열은 열처리 온도 $500^{\circ}C$에서 가장 높은 값을 나타내었다. 열처리 온도가 증가함에 따라 실리카겔 표면의 수분과 OH 작용기가 제거되어 1,2-dichlorobenzene과의 상호작용이 증가한 것으로 판단된다. 고온인 $800^{\circ}C$에서 열처리한 실리카겔은 비표면적이 감소하여 평형흡착상수와 흡착열, 모두 감소한 것으로 사료된다. 모멘트 해석으로 계산된 축분산 계수는 $0.046{\times}10^{-4}{\sim}1.033{\times}10^{-4}m^2/sec$였으며 기공 내의 확산계수는 $500^{\circ}C$ 열처리 실리카겔에서 가장 낮은 것으로 나타났다.

• 한국진공학회:학술대회논문집
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• 한국진공학회 2016년도 제50회 동계 정기학술대회 초록집
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• pp.430.1-430.1
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• 2016

We present the concept of reducible fugitive material that conformally surrounds core Cu nanowire (NW) to fabricate transparent conducting electrode (TCE). Reducing atmosphere can corrodes/erodes the underlying/surrounding layers and might cause undesirable reactions such impurity doing and contamination, so that hydrogen-/forming gas based annealing is impractical to make device. In this regards, we introduce novel reducible shell conformally surrounding indivial CuNW to provide a protection against the oxidation when exposed to both air and solvent. Uniform copper lactate shell formation is readily achievable by injecting lactic acid to the CuNW dispersion as the acid reacts with the surface oxide/hydroxide or pure copper. Cu lactate shell prevents the core CuNW from the oxidation during the storage and/or film formation, so that the core-shell CuNW maintains without signficant oxidation for long time. Upon simple thermal annealing under vacuum or in nitrogen atmosphere, the Cu lactate shell is easily decomposed to pure Cu, providing an effective way to produce pure CuNW network TCE with typically sheet resistance of $19.8{\Omega}/sq$ and optical transmittance of 85.5% at 550 nm. Our reducible copper lactate core-shell Cu nanowires have the great advantage in fabrication of device such as composite transparent electrodes or solar cells.

• 한국입자에어로졸학회지
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• 제7권3호
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• pp.79-85
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• 2011

Porous $TiO_2-SiO_2$ particles were synthesized by co-assembly of nanoparticles of $TiO_2$ and $SiO_2$ in evaporating aerosol droplets. Poly styrene latex (PSL) particles were employed as a template of porous particles. Flowrate of dispersion gas, weight ratio of $TiO_2/SiO_2$ and $SiO_2$ concentration in the precursor, and PSL size were chosen as process variables. The morphology, crystal structure, chemical bonding, and pore size distribution were analyzed by FE-SEM, XRD, FT-IR, BET. The morphology of porous $TiO_2-SiO_2$ particles was spherical and the average particle size range were from 1 to $10{\mu}m$. The particles were composed of meso and macro pores. The average particle diameter and pore volume of the as prepared particles were dependant on process variables. It was found that UV-Vis absorption of the porous particles was comparable with pure $TiO_2$ nanoparticles even though $TiO_2/SiO_2$ ratio is low in the porous particles.