• Journal of Astronomy and Space Sciences
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• 제21권4호
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• pp.243-248
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• 2004

FUSE(Far Ultraviolet Spectroscopic Explorer)를 이용해 7개의 초기형 별 방향에 존재하는 CO 흡수선을 관측했다. BEFS(Berkeley Extreme and Far-ultraviolet Spectrometer)로 관측한 54개의 초기형 별들 중에서 이번 논문에서는 시선방향으로 1개의 성간운만 존재하는 7개의 별(HD 37903, HD 97991, HD 149881, HD 156110, HD 164794, HD 214080, HD 219188)들을 선택해서 분석했다. CO 분자의 분석을 위해 자외선 영역에서 수소분자의 흡수선에 의해 가려지지 않는 E-X(0-0)($1076{\AA}$) 흡수선이 있는지 확인했으며 그 결과 3개의 별 방향에 존재하는 성간운에 대해서 CO 흡수선이 있는 것을 발견했다. 그 흡수선의 분석을 통해 성간운에 존재하는 CO의 기둥밀도를 구했고, 이번 논문에서의 결과와 이전에 구했던 수소분자의 기둥밀도로부터 CO분자와 수소분자 사이의 비율(CO to $H_2$ ratio)을 계산할 수 있었다.

• Wind and Structures
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• 제12권5호
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• pp.441-455
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• 2009

Studying the spatial distribution in coherent fields such as turbulence and turbulence-induced force is important to model and evaluate turbulence-induced forces and response of structures in the turbulent flows. Turbulence field-based coherence function is commonly used for the spatial distribution characteristic of the turbulence-induced forces in the frequency domain so far. This paper will focus to study spectral coherent structure of the turbulence and induced forces in not only the frequency domain using conventional Fourier transform-based coherence, but also temporo-spectral coherence one in the time-frequency plane thanks to wavelet transform-based coherence for better understanding of the turbulence and force coherences and their spatial distributions. Effects of spanwise separations, bluff body flow, flow conditions and Karman vortex on coherent structures of the turbulence and induced pressure, comparison between turbulence and pressure coherences as well as intermittency of the coherent structure in the time-frequency plane will be investigated here. Some new findings are that not only the force coherence is higher than the turbulence coherence, the coherences of turbulence and forces depend on the spanwise separation as previous studies, but also the coherent structures of turbulence and forces relate to the ongoing turbulence flow and bluff body flow, moreover, intermittency in the time domain and low spectral band is considered as the nature of the coherent structure. Simultaneous measurements of the surface pressure and turbulence have been carried out on some typical rectangular cylinders with slenderness ratios B/D=1 (without and with splitter plate) and B/D=5 under the artificial turbulent flows in the wind tunnel.

• 한국위성정보통신학회논문지
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• 제10권3호
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• pp.121-126
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• 2015

본 논문에서는 원형 편파 다이버시티를 구현하기 위하여 교차형 섭동 구조에 기반을 둔 새로운 원형 편파 재구성 마이크로스트립 안테나를 제안하였다. 제안한 안테나는 우회전 원형 편파와 좌회전 원형 편파를 동시에 구현하기 위하여 링 구조 방사체와 원형 편파의 방향을 선택하기 위한 두 개의 PIN 다이오드로 구성되었다. 방사체의 대각선 한 모서리에 슬롯 섭동과 스터브 섭동을 다이오드의 ON/OFF 상태를 조절함으로써, 제안한 안테나의 재구성 원형 편파는 잘 동작되고 또한 교차할 수 있었다. 또한 위성 통신 시스템 동작을 위하여 2.4 GHz의 S 대역에서 제안한 안테나는 이론적으로 분석하였고, 실험적으로 검증하였다. 제작된 안테나의 모의실험과 측정실험결과는 반사계수, 축비, 안테나 이득, 및 방사패턴에서 잘 일치함을 확인하였다.

• 한국수산과학회지
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• 제35권3호
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• pp.207-215
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• 2002

Ocean color properties can be quantified by the relationship between the band ratios of the sensor on the ocean color satellites and the measured field ocean color parameters, A tool to determine the abundance of primary organism using the observed ocean color properties from satellite is presented. Coincident to ocean color satellite passes over the Korean waters, the research vessels were deployed to survey the East Sea, the South Sea and the West Sea around the Korean waters, We have been able to have more than 101) data sets containing coincident in situ chlorophyll a and the estimated chlorophyll a derived from SeaWiFS (Sea-viewing Wide Field-of-view Sensor) from february, 1999 to October, 2001. We were able to develop three proper regional algorithms for the East Sea, the South Sea and the West Sea of the Korean peninsula to estimate chlorophyll a, and set up regional algorithms to quantify the suspended solid in the southern sea of the Korean peninsula, Futhermore we were successful in finding out a simple way of estimating chlorophyll a in the turbid water (Case 2 water) using the relationship between in situ chlorophyll a and the estimated chlorophyll a from the processed level 2 data, using the NASA's global algorithm.

• 한국재료학회지
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• 제21권4호
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• pp.192-195
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• 2011

The electro-deposition of compound semiconductors has been attracting more attention because of its ability to rapidly deposit nanostructured materials and thin films with controlled morphology, dimensions, and crystallinity in a costeffective manner (1). In particular, low band-gap $A_2B_3$-type chalcogenides, such as $Sb_2Te_3$ and $Bi_2Te_3$, have been extensively studied because of their potential applications in thermoelectric power generator and cooler and phase change memory. Thermoelectric $Sb_xTe_y$ films were potentiostatically electrodeposited in aqueous nitric acid electrolyte solutions containing different ratios of $TeO_2$ to $Sb_2O_3$. The stoichiometric $Sb_xTe_y$ films were obtained at an applied voltage of -0.15V vs. SCE using a solution consisting of 2.4 mM $TeO_2$, 0.8 mM $Sb_2O_3$, 33 mM tartaric acid, and 1M $HNO_3$. The stoichiometric $Sb_xTe_y$ films had the rhombohedral structure with a preferred orientation along the [015] direction. The films featured hole concentration and mobility of $5.8{\times}10^{18}/cm^3$ and $54.8\;cm^2/V{\cdot}s$, respectively. More negative applied potential yielded more Sb content in the deposited $Sb_xTe_y$ films. In addition, the hole concentration and mobility decreased with more negative deposition potential and finally showed insulating property, possibly due to more defect formation. The Seebeck coefficient of as-deposited $Sb_2Te_3$ thin film deposited at -0.15V vs. SCE at room temperature was approximately 118 ${\mu}V/K$ at room temperature, which is similar to bulk counterparts.

• 대한기계학회논문집B
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• 제29권2호
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• pp.263-270
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• 2005

An experimental study was performed to investigate the effects of partially premixing, varying the equivalence ratios from $0.79{\sim}{\infty}$, on NOx emissions and chemiluminescence of excited $OH^{\ast},\;CH^{ast}\;C_2^{\ast}$ radicals in laminar partially premixed flames. the signal from the electronically excited state of $OH^{\ast},\;CH^{ast}\;C_2^{\ast}$ was detected through a band pass filter with a photo multiplier tube, which are processed to the intensity ratio ($C_2^{\ast}/CH^{\ast},\;C_2^{\ast}/OH^{\ast},\;and\;CH^{\ast}/OH^{\ast}$) to reveal the correlation with local equivalence ratio. And measurements of NOx emission were made to investigate the relationship between visible flame appearance, chemiluminescence, and EINOX. The results demonstrated that (1) the flames at ${\phi}<1.59$ exhibited classical double flame structure, at ${\phi}>4.76$, the flames exhibited diffusion flame structure, and the intermediate flames at $1.59<{\phi}<4.76$ was a merged flame, (2) the $OH^{\ast}$ peak was located inside the $CH^{\ast}\;and\;C_2^{\ast}$ radical for all measured conditions and the emission intensity ratio of $C_2^{\ast}/CH^{\ast}\;and\;C_2^{\ast}/OH^{\ast}$ were identified as good marker for local equivalence ratio over a range of ${\phi}=0.79{\sim}1.2\;and\;CH^{\ast}/OH^{\ast}\;is\;0.79<{\phi}<1.9$. However, it was difficult to predict the equivalence ratio in partially premixed flames using this system for ${\phi}>2.38$, (3) the minimum NOX emission index (EINOx) is obtained for a equivalence ratio of 3.19 in the intermediate flames.

• 천문학회지
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• 제41권5호
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• pp.121-137
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• 2008

We present optical and near-infrared imaging and long-slit spectroscopy for the blue compact dwarf galaxy (BCD) Mrk 49 in the Virgo Cluster. The surface brightness distribution analysis shows that Mrk 49 consists of an off-centered blue bright compact core of r = 10" and a red faint outer exponential envelope. The $H_{\alpha}$ image and color difference suggest that these two components have different stellar populations: a high surface brightness population of massive young stars and an underlying low surface brightness population of older stars. The redder near-infrared colors of the inner most region suggest that the near-infrared flux of Mrk 49 originates from evolved massive stars associated with the current star-forming activity. The total apparent magnitude is $B_T\;=\;14.32$ mag and the mean effective surface brightness is ${\mu}_{eff}(B)\;=\;21.56$ mag $arcsec^{-2}$. Long-slit spectroscopy shows that Mrk 49 rotates apparently as a solid body within r = 10" in a plane at position angle 55 degrees with an amplitude of about $20\;km\;sec^{-1}$. The measured radial velocity of Mrk 49 was derived as $1,535\;km\;sec^{-1}$; and the total mass of stars and gases is in the range of 3 to $6\;{\times}\;10^9\;M_{\odot}$. The mass-to-light ratios for the central region of Mrk 49 in I and B band are estimated 1.0 and 0.5, respectively. The upper limit of the dark matter to visible matter ratio seems to be < 5. The oxygen abundance is $12\;+\;\log(O/H)\;=\;8.21\;{\pm}\; 0.1$ which is about one quarter of the solar value while the relative helium abundance appears to be similar to that of the sun.

• 전자공학회논문지S
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• 제36S권12호
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• pp.34-40
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• 1999

일반적인 칼러 텔레비전 시스템에서는 색차신호의 대역제한으로 인하여 고채도 영상의 색경계 부분이 열화된다. 본 논문에서는 경계부분의 열화를 보정하기 위해 잡음의 영향을 적게 받는 변형된 색상가중 휘도복조 방식을 제안하였다. 제안 방식에서는 색차신호의 미분치와 대역제한된 휘도신호의 미분치의 비로써 색상 가중치를 구하였다. 색신호의 분리가 양호한 경우, 1차 저역통과 필터를 거친 색차신호와 휘도 신호는 이론적으로 거의 완전한 보정을 할 수 있다. 또한 잡음이 있는 화상인 경우 제안 방식으로 보정하는 과정에서 미분처리에 따른 임펄스성 잡음이 수반될 수 있으며 이를 제거하기 위한 잡음저감 방법도 함께 고려하였다. 잡음이 있는 화상을 사용한 컴퓨터 모의실험을 통해서 고채도 칼러영상의 경계영역에서 해상도의 향상과 함께 대역확장의 효과를 확인하였다.

• 한국전기전자재료학회논문지
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• 제25권4호
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• pp.298-303
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• 2012

$Y_{1-x}VO_4:Eu_x^{3+}$ red phosphors were synthesized with changing the mol ratios of $Eu^{3+}$ ions by using the solid-state reaction method. The crystalline structure of phosphors was found to be a tetragonal system with the maximum diffraction intensity at $25.02^{\circ}$. The grain particles showed the truncated hexagonal patterns with a very homogeneous size distribution at 0.05 mol of $Eu^{3+}$ ion. The excitation spectra of the phosphor ceramics were composed of a broad band centered at 303 nm and weak narrow multilines peaked in the range of 360-420 nm. The dominant emission spectrum was the strong red emission centered at 619 nm due to the $^5D_0{\rightarrow}^7F_2$ electric dipole transition. The experimental results suggest that the optimum doping mol ratio of $Eu^{3+}$ ions for preparing the red phosphors is 0.10 mol with the asymmetry ratio of 5.21.

• 한국정보통신학회논문지
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• 제16권7호
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• pp.1344-1349
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• 2012

국내 DGPS 기준국은 283.5 kHz~325 kHz 대역 주파수를 사용하여 200 bps 의 GPS 보정 신호를 MSK 방식으로 전송하고 있다. 6곳의 내륙기준국은 500 W 출력으로 80 kM 영역을 서비스하며, 11곳의 해안기준국은 300 W 전력으로 185 kM의 광역 지역에 전송된다. 내륙기준국과 해안기준국에 의해 국내 DGPS 서비스 영역은 이중 또는 삼중으로 제공될 수 있다. DGPS 기준국의 고출력 신호 전송으로 기준국간 간섭과 인접 무선국간 간섭 현상이 발생할 수 있으며, 다중서비스 영역에 위치한 사용자 단말기의 수신 성능은 간섭 영향을 받을 수 있다. 본 논문에서는 국내 DGPS 기준국에 대한 간섭 보호비를 정의하고, 중파대역 전파 모델을 통하여 기준국간 간섭과 인접무선국간 간섭영향을 분석하고 사용자 단말기의 간섭을 분석한다.