http://chineseinput.net/에서 pinyin(병음)방식으로 중국어를 변환할 수 있습니다.
변환된 중국어를 복사하여 사용하시면 됩니다.
Far-ultraviolet Observations of the Taurus-Perseus-Auriga Complex
임태호,민경욱,선광일,Lim, Tae-Ho,Min, Kyoung-Wook,Seon, Kwang-Il 한국천문학회 2012 天文學會報 Vol.37 No.2
We firstly present the unified Far-UV continuum map of the Taurus-Auriga-Perseus (TPA) complex, one of the largest local associations of dark cloud located in (l, b)=([154,180], [-28, -2]), by merging both FIMS and GALEX. The FUV continuum map shows that dust extinction correlate well with the FUV around the complex. It shows strong absorption in FUV toward the dense Taurus cloud while it does not in California cloud. It turned out that it is related to the relative location of each cloud and Perseus OB2 association. We also present some results of dust scattering simulation based on Monte Carlo Radiative Transfer technique (MCRT). Through this dust scattering simulation, we have derived the scattering parameter for this region, albedo(a)=$0.42^{+0.05}{_{-0.05}}$, asymmetry factor(g)=$0.47^{+0.11}{_{-0.27}}$. The optical parameters we obtained seem reasonable compared to the theoretical model values ~0.40 and ~0.65 for the albedo and the phase function though the phase function is rather small. Using the result of simulation, we figured out the geometries of each cloud in the complex region, especially their distances and thicknesses. Our predictions from the results are in good agreement with the previous studies related to the TPA complex. For example, the Taurus cloud is within ~200pc from the Sun and the Perseus seems to be multi-layered, at least two. The California cloud is more distant than the other cloud on average at ~350 pc and Auriga cloud seems to be between the Taurus cloud and the eastern end of the California cloud. We figured out that across the TPA complex region, there might be some correlation between the LSR velocity and the distance to each cloud in the complex.
SiO<sub>2</sub>-TiO<sub>2</sub>계 복합 나노섬유의 제조 및 광활성 연구
현동호,임태호,이성욱,Hyun, Dong Ho,Lim, Tae-Ho,Lee, Sung Wook 한국공업화학회 2008 공업화학 Vol.19 No.5
전구체로서 알콕사이드[Tetraethyl orthosilicate (TEOS), Titanium (IV) isopropoxide (TiP)]를 사용하여 졸-겔 방법으로 전기방사에 적합한 졸을 제조한 후, $(1-x)SiO_2-(x)TiO_2$계 복합 나노섬유를 제조하였다. 제조된 광활성 무기나노섬유의 표면 및 구조적 특성은 X-선회절분석(XRD), 주사전자현미경(SEM), 투과전자현미경(TEM), 열중량분석 및 미분주사칼로리미터분석 (TGA-DSC), 적외선분광분석((FT-IR)을 통하여 확인하였다. $(1-x)SiO_2-(x)TiO_2$계에서 $TiO_2$ 양이 증가하면 전기방사된 복합섬유직경은 증가하였으며, 저온에서 안정한 아나타제 $TiO_2$ 결정에서 루타일로의 상전이는 $1000^{\circ}C$에서의 열처리 후에도 고루 분산되어 있는 $SiO_2$로 인해 $0.6SiO_2-0.4TiO_2$계까지는 아나타제상으로 존재하였다. $SiO_2-TiO_2$계 복합체 나노섬유의 광활성은 메틸렌블루 광분해 실험 및 UV-vis/DRS 분석을 통해 자외선 영역에서 나타남을 확인하였다. $(1-x)SiO_2-(x)TiO_2$ composite fibers with various compositions of $TiO_2$ were prepared by electrospinning their sol-gel precursors of titanium (IV) iso-propoxide (TiP), and tetraethyl orthosilicate (TEOS). The surface morphology and structure of sintered composite fibers were characterized using X-ray diffraction (XRD), scanning electron microscopy (SEM), transmission electron microscopy (TEM), simultaneous thermogravimetric analysis-differential scanning calorimetry (TGA-DSC) and Fourier transform infrared spectroscopy (FT-IR). As the content of $TiO_2$ in $(1-x)SiO_2-(x)TiO_2$ system was increased the average diameter of composite fibers was proportionally increased. Also, the transformation of $TiO_2$ from anatase to rutile form was inhibited by the highly dispersed $TiO_2$ around $SiO_2$ particles up to $0.6SiO_2-0.4TiO_2$ composite fibers even after calcination at $1000^{\circ}C$. The photocatalytic activity of $SiO_2-TiO_2$ composite fibers was examined for the methylene blue (MB) decomposition which was confirmed using UV-vis/DRS spectra. The experiments demonstrated that the MB in aqueous solution was successfully photodegraded using $SiO_2-TiO_2$ composite nanofibers under UV-visible light irradiation.
대한민국 남해 해역에서 원형 배열 하이드로폰을 이용한 수중 OFDM 시스템의 적응 빔포밍 연구
김준호(Jun Ho Kim),차민혁(Min Hyuk Cha),왕비(Fei Wang),임태호(Tae Ho Im),고학림(Hak Lim Ko) 한국통신학회 2021 한국통신학회 학술대회논문집 Vol.2021 No.11
본 논문은 12개의 하이드로폰을 원형으로 배열하여 하이드로폰 개수에 따른 수중 OFDM 시스템의 MMSE 빔포밍 성능향상 실험을 수행하였다, 대한민국 경상남도 거제도 인근 해역에서 실해역 실험을 진행하였으며, 실해역 실험 데이터를 통해 원형 배열 하이드로폰의 개수를 3개, 4개, 6개, 12개로 달리하여 MMSE 빔포밍을 적용한 결과 omni대비 최대 8.5392dB의 EVM 이득이 확인되었으며, BER이 최대 0.0285 낮아졌음을 확인하였다.
Simulation study of dust-scattered Far-Ultraviolet emission in the Orion-Eridanus Superbubble
조영수,민경욱,임태호,선광일,Jo, Young-Soo,Min, Kyoung-Wook,Lim, Tae-Ho,Seon, Kwang-Il 한국천문학회 2012 天文學會報 Vol.37 No.2
We present the results of dust scattering simulations carried out for the Orion-Eridanus Superbubble region by comparing them with observations made in the far-ultraviolet. The albedo and the phase function asymmetry factor (g-factor) of interstellar grains were estimated, as were the distance and thickness of the dust layers. The results are as follows: [0.43]_(-0.04)^(+0.02) for the albedo and [0.43]_(-0.2)^(+0.2) for the g-factor, in good agreement with previous determinations and theoretical predictions. The distance of the assumed single dust layer, modeled for the Orion Molecular Cloud Complex, was estimated to be ~110 pc, and the thickness ranged from ~130 at the core to ~50 pc at the boundary for the region of present interest, implying that the dust cloud is located in front of the superbubble. The simulation result also indicates that a thin (~10 pc) dust shell surrounds the inner X-ray cavities of hot gas at a distance of ~70-90 pc.