• 한국전기전자재료학회:학술대회논문집
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• 한국전기전자재료학회 1997년도 춘계학술대회 논문집
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• pp.8-11
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• 1997

This study makes SrTiO$_{3}$ with nonpolarity among ferroelectrics by RF sputtering as dielectric layer, produces thin film of Si/SrTiO$_{3}$ and Si/Ti/SrTiO$_{3}$ of MOS structure using Ti as buffer layer, measures and examines the electrical features with optical refractive index, absorption rate, permittivity, photon energy and as a result, ferroelectrics oscillation occurrs by the interaction within a film by light temperature and the absorption of thin film with Ti as buffer layer is increased. It is found that the pea\ulcorner of permittivity value of Ti/SrTiO$_{3}$ thin film has low values and is appeared late and as dipole which is found in dielectric is shown, the experiment satisfies the theory In the nature of permittivity by photon energy, imaginary value is higher and current variation slope of thin film of thickness SrTiO$_{3}$ has lower values in reverse bias.

• 천문학회보
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• 제39권2호
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• pp.47.1-47.1
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• 2014

The calcium infrared triplet (CaT) is one of the prominent absorption features in the infrared wavelength regime. Recently, this absorption feature has been getting attention in the prediction of metallicity of stellar populations because of its strong sensitivity to the calcium abundance and metallicity of a star. However, we find that measuring metallicity directly from CaT is very dangerous because the formation mechanism of CaT is very inefficient in the cool stars which are abundant in metal-rich populations. This characteristics of CaT make the CaT-metallicity relation to converge around ~ $8{\AA}$ in the metal-rich regime. Our results suggest that, because of the converging CaT-metallicity relation in the metal-rich regime, the metallicity of simple stellar populations greater than [Fe/H]~-0.5 is unreliable when the linear conversion between CaT and metallicity is applied to derive metallicity. Based on these results, we suggest that CaT is not a good metallicity indicator for the metal-rich stellar populations.

• 천문학회보
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• 제41권1호
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• pp.36.1-36.1
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• 2016

The physical scenario describing the origin of quasar winds remains largely unsettled due to our failure to account for X-ray weak BAL quasars. We approach this problem by studying the relation between the inner part of the outflow which is likely to be shielding the X-ray emission and thereby helping to drive the UV winds characterised by broad absorption lines (BALs). In particular, we aim to probe the wind-shield connection in the highly X-ray variable BAL quasar PG 2112+059, which has exhibited periods of X-ray weakness and X-ray normality in the past. A set of two 20 ks Chandra observations and two contemporaneous HST observations, separated by at least eight months, combined with a nearly simultaneous archival Chandra-HST observation from 2002, afford us a unique opportunity to study the connection between the shield (which is thought to be responsible for the X-ray absorption) and the ionisation state of the wind (observed as UV BAL features; e.g., C IV and O VI lines) over various timescales.

• 한국전기전자재료학회논문지
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• 제16권2호
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• pp.89-96
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• 2003

Photoluminescence (PL) and photoluminescence excitation (PLE) spectroscopy have been performed at 6 K on the 1540 nm $^4$I$\_$(13/2)/\longrightarrow$^4$I$\_$(15/2)/ emission of Er$\^$+3/ in in situ Er-doped GaN The PL and PLE spectra of in situ Er-doped GaN are compared with those of Er-implanted GaN in this study. The lineshapes of the broad PLE absorption bands and the broad PL bands in the spectra of the in situ Er-doped GaN are similar to those in Er-doped glass rather than in the Er-implanted GaN. The PL spectra of this in situ Er-doped GaN are independent of excitation wavelength and their features are significantly different from the site-selective PL spectra of the Er-implanted GaN. These PL and PLE studies reveal that a single type of Er$\^$3+/ sites is present in the in situ Er-doped GaN and these Er sites are different from those observed in the Er-implanted GaN. In addition, the comparison of the PL single strength illustrates that the excitation of Er$\^$3+/ sites through the energy absorption of defects in Er-implanted GaN.

• 대한원격탐사학회지
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• 제23권6호
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• pp.493-500
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• 2007

일반적으로 분광측정을 수행함에 있어서 측정 대상물, 측정 방법, 측정 조건 등에 따라서 측정 결과가 상이하게 나타난다. 본 연구에서는 광물 및 암석 샘플의 전처리, 센서와 대상물과의 거리에 대한 표준화 방법을 제시하고, 납석의 분광특성 연구를 수행하였다. 광물, 암석 샘플의 크기는 노두의 규모와 상태에 따라서 다양하기 때문에 샘플과 센서간의 거리를 일정하게 유지하는 것이 중요하다. 표준화를 수행하기 전에 동일한 암석(석영반암)에 대해서 자연석, 자갈, 분말 그리고 절단암 등 다양한 샘플을 준비하였다. 샘플의 표면 상태와 그림자의 영향을 최소화하고 정량적인 분석을 위하여 센서와 샘플간의 거리를 30cm로 유지하고 $1{\sim}2cm$ 두께의 절단암을 3회 반복 측정하였다. 제안된 방법을 검증하기 위해서 납석에 대한 사례 연구를 수행하였다. 본 연구결과에 따르면 납석은 1.406nm, 1,868nm, 2.180nm 그리고 2.180nm 파장대역에서 강한 흡수 양상을 보이며, 특히 1.406nm와 2.180nm 파장대역에서 강한 흡수가 일어난다. 이러한 흡수 특징은 Landsat TM 영상의 밴드 7과 ASTER 영상의 밴드 8과 일치한다. 따라서, 이러한 결과를 이용하여 육안으로 구분되지 않은 다른 대상물(나지, 주차장, 채석장 등)과 납석 광산을 구분할 수 있다.

• 한국결정성장학회지
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• 제19권2호
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• pp.90-94
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• 2009

Mong Hsu rubies from Myanmar were heat treated in oxidizing(oxygen) atmosphere at $1650^{\circ}C$ for 1 hour. The investigations of the micro-structural defects in the samples before and after heat treatment have been carried out by the variety of analysis techniques of FTIR, UV-VIS-NIR and SEM-EDS. It was found that after heat treatment the dark blue cores region were disappeared and turned to orange red color with the presence of the dense cloudy brownish colored tiny particles in and near former blue zoning. As-received ruby samples only revealed the presence of FTIR absorption peaks of diaspore, boehmite and O-H stretching, at 1986, 2115 and $3078/3319\;cm^{-1}$ respectively. The UV-VIS-NIR absorption of as-received and heat treated ruby samples similarly showed peaks at 405, 554 and 693 nm associated with $Cr^{3+}$, but for the same samples, the absorption peak of heat-treated ruby samples at 693 nm was somewhat stronger than that of the untreated ruby samples. Especially the presence of $Cr^{3+}$ peaks at 659 and 675 nm was found obviously in as-received ruby samples only. The SEM-EDS investigation disclosed the micro-porous defect structures commonly related to the core regions of the untreated ruby samples, which after heat treatment in an oxidizing environment those defect features have been dissolved into the host phase resulting in the lightening or disappearance of the dark coloration of ruby core.

• 한국진공학회:학술대회논문집
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• 한국진공학회 2013년도 제44회 동계 정기학술대회 초록집
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• pp.398-398
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• 2013

The electronic properties and the local structure of tantalum oxide thin film with variation of oxygen flow rate ranging from 9.5 to 16 sccm (standard cubic centimeters per minute) have been investigated by X-ray photoelectron spectroscopy (XPS), Reflection Electron Energy Loss Spectroscopy (REELS), and X-ray absorption spectroscopy (XAS). The XPS results show that the Ta4f spectrum for all films consist of the strong spin-orbit doublet $Ta4f_{7/2}$ and $Ta4f_{5/2}$ with splitting of 1.9 eV. The oxygen flow rate of the film results in the appearance of new features in the Ta4f at binding energies of 23.2 eV, 24.4 eV, 25.8, and 27.3 eV, these peaks attribute to $Ta^{1+}$, $Ta^{2+}$, $Ta^{4+}$/$Ta^{2+}$, and $Ta^{5+}$, respectively. Thus, the presence of non-stoichiometric state from tantalum oxide ($TaO_x$) thin films could be generated by the oxygen vacancies. The REELS spectra suggest the decrease of band gap for tantalum oxide thin films with increasing the oxygen flow rate. The absorption coefficient ${\mu}$ and its fine structure were extracted from the fluorescence mode of extended X-ray absorption fine structure (EXAFS) spectra. In addition, bond distances (r), coordination numbers (N) and Debye-Waller factors (${\sigma}^2$) each film were determined by a detailed of EXAFS data analysis. EXAFS spectrapresent both the increase of coordination number of the first Ta-O shell and a considerable reduction of the Ta-O bond distance with the increase of oxygen flow rate.

• Macromolecular Research
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• 제12권3호
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• pp.322-324
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• 2004

Poly(1-dodecyl-2,5-pyrrylene vinylene) (PDPV) has an extended 1t-conjugated structure and exhibits characteristic spectroscopic features. The PDPV we prepared has an absorption maximum at 510nm and its long absorption tail at ca. 750nm in methylene chloride is due to the long 1t-conjugated system connected to vinyl group. The large red-shift of emission was 625nm upon excitation at 480nm, which suggests the existence of a low emissive state. The emission of PDPV in less-polar solvents decreased markedly relative to that in the more-polar solvents; this observation was ascribed possibly to quenching by a strong vibrational mode of the dodecyl groups of PDPV in less-polar solvents. Furthermore, the emission from the high-energy side had a single decay component (0.1㎱, 49.96%), while that from the low-energy side had two components (0.6㎱, 27.1 %; 2.7㎱, 22.87%). We characterized the redox properties of PDPV by cyclic voltammetry. Every redox peak showed irreversible behavior; the oxidation peaks appeared at 1.7,0.8, and 0.6V and the reduction peak at -0.5V.

• 폴리머
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• 제34권4호
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• pp.376-380
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• 2010

분자내 전하이동(intramolecular charge transfer, ICT)이 가능한 도너-$\pi$-억셉터(D-$\pi$-A)타입의 발색단 을 근간으로 한 폴리머를 신규 합성하였다. 이 폴리머는 UV-visible spectra 측정결과 용액 상태에서 뿐만 아니라 고체박막 상태에서도 카르보닐기(carbonyl group)에서 기인하는 흡수와 함께 ICT에 의한 장파장 영역에서의 흡수가 관 찰되었다. $Eu^{3+}$ 이온의 첨가에 의해 장파장영역에서 일어나는 흡수의 적색이동(red shift)을 유도하였으며, 더불어 용 액과 박막의 색상도 황색에서 적색으로 변화하는 것이 관찰되었다. 합성된 고분자의 형태 및 유기 용매에 대한 용해도 는 가교제의 함량에 따라 다양한 특성을 나타내었다. 또한, 첨가된 가교제의 함량과 $Eu^{3+}$ 이온의 첨가는 성막 특성의 향상을 유도하였다.

• 한국광물학회지
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• 제30권1호
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• pp.31-43
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• 2017

본 연구는 백화현상이 극명하게 발생한 미인폭포 내 백색침전물을 대상으로 X선형광분석법, X선회절분석법 및 휴대용 분광계를 이용하여 광물조성을 확인하고, 분광특성을 고찰하였다. 그 결과 모든 시료에서 알루미늄이 평균농도보다 높게 검출되었고, 대부분의 시료에서 카드뮴과 니켈의 오염도가 높았다. X선회절분석 결과 모든 시료에서 석영, 고령토, 롬보클레이스, 알루미노코큠바이트, 깁사이트의 광물이 검출되었고 중금속은 점토광물에 흡착하여 존재한다고 판단된다. 백색침전물의 분광학적 특성은 가시광선 대역에서 반사도가 증가하는 추세를 보이나, 근적외선, 단파적외선으로 파장이 길어짐에 따라 반사도가 서서히 감소한다. 백색침전물의 흡광특성을 바탕으로 볼 때 분광학적 특성은 고령토, 롬보클레이스, 알루미노코큠바이트, 깁사이트에 의해 발생하는 것으로 판단된다. 퇴적물 내 중금속 종류 및 함량에 따른 영역별 흡광깊이 변이양상을 분석한 결과, Al-OH의 흡광특성인 2202 nm에서 알루미늄함량과 흡광깊이 사이에 높은 양의 상관관계가 성립하는 것이 확인되었다. 이는 분광학적 특성 중 흡광깊이가 중금속 함량의 유추에 유용할 수 있음을 지시한다.