• 센서학회지
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• 제2권1호
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• pp.101-108
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• 1993

컬러센서를 위한 $TiO_{2}$/Se : Te 이종접합을 고주파 반응성 스퍼터링법과 진공증착법을 이용하여 제작하였다. 제조된 $TiO_{2}$ 막형성의 최적조건은 $1000{\AA}$의 $TiO_{2}$ 두께에서 고주파전력 120 W, 기판온도 $100^{\circ}C$, 산소농도 50% 및 분위기압 50 mTorr였다. 이 때 광투과율은 파장 550 nm에서 85%, 저항률은 $2{\times}10^9{\Omega}{\cdot}cm$, 굴절률은 2.3이었다. 제조된 $TiO_{2}$막은 직접천이형 에너지 밴드구조를 가지며 광학적 밴드갭은 3.58 eV였다. 제조된$TiO_{2}$막을 $400^{\circ}C$에서 30분간 열처리함으로써 광투과율이 파장 $300{\sim}580$ nm범위에서 $0{\sim}25%$까지 개선되었다. 또한 화학양론적 조성비를 조사하기 위하여 AES 분석을 한 결과 Ti 및 0의 조성비는 1 : 1.7로 나타났다. 한편 Se : Te 막형성의 최적조건은 $190^{\circ}C$에서 1분간 열처리했을 때였다. 이러한 조건으로 제조된 Se : Te막의 광학적 밴드갭은 1.7 eV였으며 육방정계구조의 (100) 방향 및 (110) 방향으로 Se : Te 막이 결정화됨을 알 수 있었다. 1000 lux의 조도에서 Se : Te막의 광전변환률은 0.75였다. 또한 Se에 Te를 첨가함으로써 장파장영역의 분광감도가 향상되었다. $TiO_{2}$/Se : Te 이종접합의 분광감도는 가시광 전영역에서 비교적 넓은 분광감도를 나타내었으며, 특히 청색영역에서 a-Si박막보다 우수한 분광감도를 나타내었다.

• Journal of Astronomy and Space Sciences
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• 제36권1호
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• pp.21-33
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• 2019

This paper focuses on the interpretation of radiation fluxes from active galactic nuclei. The advantage of positron annihilation spectroscopy over other methods of spectral diagnostics of active galactic nuclei (therefore AGN) is demonstrated. A relationship between regular and random components in both bolometric and spectral composition of fluxes of quanta and particles generated in AGN is found. We consider their diffuse component separately and also detect radiative feedback after the passage of high-velocity cosmic rays and hard quanta through gas-and-dust aggregates surrounding massive black holes in AGN. The motion of relativistic positrons and electrons in such complex systems produces secondary radiation throughout the whole investigated region of active galactic nuclei in form of cylinder with radius R= 400-1000 pc and height H=200-400 pc, thus causing their visible luminescence across all spectral bands. We obtain radiation and electron energy distribution functions depending on the spatial distribution of the investigated bulk of matter in AGN. Radiation luminescence of the non-central part of AGN is a response to the effects of particles and quanta falling from its center created by atoms, molecules and dust of its diffuse component. The cross-sections for the single-photon annihilation of positrons of different energies with atoms in these active galactic nuclei are determined. For the first time we use the data on the change in chemical composition due to spallation reactions induced by high-energy particles. We establish or define more accurately how the energies of the incident positron, emitted ${\gamma}-quantum$ and recoiling nucleus correlate with the atomic number and weight of the target nucleus. For light elements, we provide detailed tables of all indicated parameters. A new criterion is proposed, based on the use of the ratio of the fluxes of ${\gamma}-quanta$ formed in one- and two-photon annihilation of positrons in a diffuse medium. It is concluded that, as is the case in young supernova remnants, the two-photon annihilation tends to occur in solid-state grains as a result of active loss of kinetic energy of positrons due to ionisation down to thermal energy of free electrons. The single-photon annihilation of positrons manifests itself in the gas component of active galactic nuclei. Such annihilation occurs as interaction between positrons and K-shell electrons; hence, it is suitable for identification of the chemical state of substances comprising the gas component of the investigated media. Specific physical media producing high fluxes of positrons are discussed; it allowed a significant reduction in the number of reaction channels generating positrons. We estimate the brightness distribution in the ${\gamma}-ray$ spectra of the gas-and-dust media through which positron fluxes travel with the energy range similar to that recorded by the Payload for Antimatter Matter Exploration and Light-nuclei Astrophysics (PAMELA) research module. Based on the results of our calculations, we analyse the reasons for such a high power of positrons to penetrate through gas-and-dust aggregates. The energy loss of positrons by ionisation is compared to the production of secondary positrons by high-energy cosmic rays in order to determine the depth of their penetration into gas-and-dust aggregations clustered in active galactic nuclei. The relationship between the energy of ${\gamma}-quanta$ emitted upon the single-photon annihilation and the energy of incident electrons is established. The obtained cross sections for positron interactions with bound electrons of the diffuse component of the non-central, peripheral AGN regions allowed us to obtain new spectroscopic characteristics of the atoms involved in single-photon annihilation.

• 한국지리정보학회지
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• 제25권1호
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• pp.101-119
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• 2022

기존의 녹조 모니터링은 현장 채수에 의한 국지적인 조사로 인해 녹조 발생 및 확산 규모 등에 대한 공간적 분포 파악에 한계가 있다. 이에 본 연구에서는 무인항공기 및 다중분광센서를 이용하여 녹조 모니터링을 수행하고, 녹조 분포 현황 자료를 산출하고자 하였다. 조류 우심구간인 낙동강 하류에 위치한 물금·매리 구간을 대상으로 현장조사 및 다중분광영상 촬영을 수행하였다. 현장 채수 시료의 Chlorophyll-a(Chl-a) 값과 분광지수(Spectral Index)들의 상관관계로 도출한 Chl-a 추정식을 비교 분석하였다. 그 결과 분광지수 중 Maximum Chlorophyll Index(MCI)가 가장 높은 통계적 유의성(R²=0.91, RMSE=8.1mg/m³)을 나타냈다. Chl-a 농도가 가장 높은 2021년 08월 05일 영상에 MCI를 적용하여 녹조 분포 지도를 작성하였고, 이로부터 산출한 수계 면적은 1.7km²이며, 조류경보제 발령 단계 중 경계(Warning) 면적은 1.03km²(60.56%), 대발생(Algal Bloom) 면적은 0.67km²(39.43%)를 나타내었다. 또한 연구기간 동안(2021년 07월 01일~2021년 11월 01일) 취득된 영상 내 "경계" 이상에 해당하는 영역에 대한 발생 일수를 계산한 결과, 하천 전 구간에서 최소 12회에서 최대 19회까지 "경계" 이상의 Chl-a 농도가 관측되었다. 본 연구에서 산출한 다중분광영상의 Chl-a 농도와 녹조발생지수는 녹조에 대한 공간적 분석이 용이하므로 조류경보제와 같은 현장 채수 위주의 지점 단위 자료를 보완할 수 있을 것으로 기대된다.

• Journal of Microbiology and Biotechnology
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• 제8권5호
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• pp.455-460
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• 1998

In the course of screening for new antitumor substances, a novel cytotoxic agent inducing apoptotic cell death was isolated from the culture broth of marine bacterial strain SCRC A-20. Strain SCRC A-20 was separated from a mollusk and was chemotaxonomically identified as a Streptomyces sp. The cytotoxic substance was purified by organic solvent extraction followed by silica gel column chromatography and preparative TLC. HRFAB-MS determined its molecular formula to be $C_{30}H_{40}N_2O_5$ (MW 508). The 1D and 2D NMR spectral data demonstrated that the substance has a novel lactam structure of a 20-membered macrocycle coupled with a unique acyl tetramine and bicyclo［3.3.0］ octane, which includes three methyl groups, six olefinic protons, five carbonyl groups, a conjugated diene and a dienone. The substance, named aburatubolactam C, appeared to be cytotoxic for various continuously proliferating tumor cells of human and murine origins. The $IC_{50}$ values determined by MIT assay were in the range of 0.3 to $5.8\mug/ml$. When Jurkat T cells were treated with $3\mug/ml$. of aburatubolactam C, the apoptotic DNA fragmentation was detectable within 3 h, indicating that the cytotoxic effect of aburatubolactam C on tumor cells is attributable to the induced apoptosis.

• 한국지진공학회논문집
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• 제16권3호
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• pp.35-42
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• 2012

암반지반에 주어진 등재해도 스펙트럼에 상응하는 원전부지 토사지반에서의 등재해도 스펙트럼을 도출하기 위한 확률론적 방법론을 제시하였다. 이를 위해 지진 운동 및 지반의 불확실성을 고려한 지반응답 해석을 통해 토사지반 지표에서의 지진동 증폭계수를 산정하였다. 증폭계수는 가장 상관관계가 높은 지반운동의 스펙트럴 가속도 규모와의 회귀분석을 통해 계산되었다. 이 방법론을 적용하여 국내 KNGR (Korean Next Generation Reactor) 및 APR1400 (Advanced Power Reactor 1400) 원전의 포괄부지 지반 중 B1, B4, C1 및 C3 지반을 대상으로 등재해도 스펙트럼을 도출하였다. 등재해도 스펙트럼을 통해 지진동 발생 빈도 별 위험 주파수 대역을 평가하고 분석하였다. 이 결과는 원전의 종합적 지진리스크 평가 결과를 보다 합리적으로 개선하는 데에 활용될 수 있으며, 향후 다양한 종류의 토사지반에 대한 등재해도 스펙트럼을 평가하는 데에 적용할 수 있을 것으로 기대된다.

• Structural Engineering and Mechanics
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• 제33권1호
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• pp.79-93
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• 2009

This paper investigates the possibility of controlling the response of typical portal frame structures to blast loading using a combination of semi-active and passive control devices. A one storey reinforced concrete portal frame is modelled using non-linear finite elements with each column discretised into multiple elements to capture the higher frequency modes of column vibration response that are typical features of blast responses. The model structure is subjected to blast loads of varying duration, magnitude and shape, and the critical aspects of the response are investigated over a range of structural periods in the form of blast load response spectra. It is found that the shape or length of the blast load is not a factor in the response, as long as the period is less than 25% of the fundamental structural period. Thus, blast load response can be expressed strictly as a function of the momentum applied to the structure by a blast load. The optimal device arrangements are found to be those that reduce the first peak of the structural displacement and also reduce the subsequent free vibration of the structure. Semi-active devices that do not increase base shear demands on the foundations in combination with a passive yielding tendon are found to provide the most effective control, particularly if base shear demand is an important consideration, as with older structures. The overall results are summarised as response spectra for eventual potential use within standard structural design paradigms.

• 천문학회보
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• 제40권1호
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• pp.78.3-78.3
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• 2015

About 70 high redshift quasars with $z{\geq}5$ have been discovered through combinations of standard broad-band filters to distinguish them from contaminating sources. However, among the discovered quasars so far, there is a redshift gap at $5{\leq}z{\leq}6$ due to the limitation of traditional filter sets and selection techniques. To understand the early mass growth of supermassive black holes and the final stage of the cosmic reionization, it is important to find a statistically meaningful sample of quasars with various physical properties. Here we suggest a new selection technique of high redshift quasars using medium-band filters: nine filters with bandwidths of 50nm and central wavelengths from 625 to 1025nm. Photometry with these medium-bands traces the spectral energy distribution (SED) of a source, similar to spectroscopy with R~15. We installed these filters to SED camera for QUasars in EArly uNiverse (SQUEAN) on the 2.1m telescope at McDonald Observatory, and conducted test observations of known high redshift quasars at $4.7{\leq}z{\leq}6.1$ and also dwarf stars for comparison. We found differences in SED shapes between high redshift quasars and dwarf stars, determined their locations on color-color diagrams, and demonstrated that the medium-band filters can enhance the efficiency of selecting robust quasar candidates in this redshift range. In this poster, we propose an effective selection method of high redshift quasars using these medium-band filters and discuss its effect on our high redshift quasar survey.

• 천문학회보
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• 제40권1호
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• pp.51.4-52
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• 2015

From 2010 to 2014, CQUEAN (Camera for QUasars in EArly uNiverse) has been operated for the observation at the 82 inch Otto Struve Telescope of the McDonald Observatory, US. This camera is optimized at wavelength range of 0.7 - 1.1 um with seven (g', r', I', z', Y, Iz and Is) broad-band filters for the survey of high redshift (z > 5) quasars in the early universe. We are upgrading this system to identify more details of SED (Spectral Energy Distribution) of quasar candidates and other astronomical sources. The SQUEAN is comprised of a focal reducer, a CCD camera, a new filter wheel, new auto guiding system and new control software. The new filter wheel consists of interchangeable cartridges for various wavelength and size of filters. 50 nm medium bandwidth filters from 600 - 1050 nm, seven SDSS (Sloan Digital Sky Survey) filters and Johnson-Cousin BVRI filters are installed for now. We also have a plan to use narrow band interference filters to classify high redshift quasars or to obtain SEDs of interesting astronomical sources in details more efficiently. We also developed KAP82 (Kyung Hee University Auto guiding Package for 82 inch telescope) for auto guiding software. CQUEAN and SQUEAN have been developed by CEOU (Center for the Exploration of the Origin of the Universe).

• Mycobiology
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• 제40권1호
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• pp.20-26
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• 2012

The complexes of tailor made ligands with life essential metal ions may be an emerging area to answer the problems of multi drug resistance. The coordination complexes of VO(II), Co(II), Ni(II) and Cu(II) with the Schiff bases derived from isatin with 3-chloro-4-floroaniline and 2-pyridinecarboxaldehyde with 4-aminoantipyrine have been synthesized by conventional as well as microwave methods. These compounds have been characterized by elemental analysis, molar conductance, electronic spectra, FT-IR, FAB mass and magnetic susceptibility measurements. FAB mass data show degradation of complexes. Both the ligands behave as bidentate and tridentate coordinating through O and N donor. The complexes exhibit coordination number 4, 5 or 6. The Schiff base and metal complexes show a good activity against the bacteria; $Staphylococcus$ $aureus$, $Escherichia$ $coli$ and $Streptococcus$ $fecalis$ and fungi $Aspergillus$ $niger$, $Trichoderma$ $polysporum$, $Candida$ $albicans$ and $Aspergillus$ $flavus$. The antimicrobial results also indicate that the metal complexes are better antimicrobial agents as compared to the Schiff bases. The minimum inhibitory concentrations of the metal complexes were found in the range 10-40 ${\mu}g/mL$.

• 한국지리정보학회지
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• 제4권4호
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• pp.72-78
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• 2001

본 연구에서는 경남 거제시 연초면 지역의 소나무재선충(Bursaphelenchus Xylophilus) 피해발생 선단지를 보다 효율적으로 추출하기 위하여 IKONOS 1m 영상의 공간해상도와 Landsat TM 영상의 band 3, 4와 동일 파장대역이면서 식생과 같은 산림분야 연구에 많이 이용되고 있는 4m 영상의 Red(0.63~0.69)밴드, NIR(0.76~0.90)밴드를 활용하였다. 그 결과 IKONOS 4m 영상의 식생밴드(NIR band)를 이용한 히스토그램 분석이 가장 효과적이었으며, 이는 GPS(global positioning system)를 이용한 현지조사에서 총 22개의 sample 지점에서 15개의 소나무재선충 피해목을 추출함으로서 확인되었다. 본 연구는 소나무재선충 피해지역 추출뿐만 아니라 산림병해충 피해연구에 대한 고해상도 위성영상의 활용가능성을 제시하고자 한다.