• Proceedings of the Korean Printing Society Conference
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• 1995.11a
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• pp.13-17
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• 1995

헤테로원자(X=O, S, Se)의 변환에 따라 용액상에서 Merocyanine색소 및 Cyanine색소의 헤테로원자X는 p궤도의 원자보다 d궤도의 원자가 공명에 관여하여 공역계확장에 기여하였고, 유전률이 큰 용매 일수륵 Merocyanine색소는 장파장으로 흡수극대치가 이동하였다. 또 Cyanine색소의 기저상태는 $I^-$이온과 정전하 발색단을 가진 이온성 화합물로 되어 있으므로 극성용매에서 $I^-$ 이온의 전하가 색소본체로 전하 이동전이가 발생하여 단파장화 하였다. 고상에서 색소의 농도가 높을 수록 색소분자간의 거리가 가까워져 색소 상호작용이 변화하여 흡수스펙트럼에서는 전체적으로 폭이 넓은 형태로 나타났으며 이것은 농도가 높을 수록 색소분자간의 거리가 가까워져 색소 상호작용이 변화한 때문이라고 생각된다. 또한 3차원 형광의 저농도에서 보이지 않는 새로운 스펙트럼이 Cyanine색소에서 나타났으며 이 스펙트럼은 색소고유의 흡수에 기인한 것으로 Eximer형광으로 생각된다. 광전특성에 있어서는 Merocyanine색소가 Cyanine색소보다 활성화에너지가 낮아 전하이동도가 커짐에 따라 높은 광전특성을 나타내었다. 그리고 Merocyanine색소 헤테로원자(X)의 비교에서 광전특성은 O

• Journal of the Korea Academia-Industrial cooperation Society
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• v.8 no.5
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• pp.1273-1278
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• 2007

In living system, various types of metal chelated protein show their intrinsic biological activities. In order to investigate the chelation reaction between protein and metal, zinc chelated peptide was systhesized by the peptide, hydrolyzed protein, with zinc. And simple analytical method fot the chelation reaction was developed using MALDI-TOF mass spectrometry.

• Korean Journal of Materials Research
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• v.9 no.12
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• pp.1229-1233
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• 1999

In this research, We fabricated Langmuir-Blodgett(LB) ultra-thin films with (N-docosyl quinolinium)- TCNQ(1:2) complex. The characteristics ${\pi}$-A isotherms were studied to find optimum conditions of deposition by varing temperature of subphase, compression speed of barrier and amount of spreading solution. Film formation was verified by measuring transfer ratio, maximum absorption of UV-vis spectra, capacitance and ellipsometry. From the results, it was concluded that the LB film formed well with molecular oder was fabricated.

• Journal of Astronomy and Space Sciences
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• v.21 no.4
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• pp.391-398
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• 2004

Far-ultraviolet Imaging Spectrograph (FIMS) is the main payload of the Korea's first scientific micro satellite STSAT-1, which was launched at Sep. 27 2003 successfully. Major objective of FIMS is observing hot gas in the Galaxy in FUV bands to diagnose the energy flow models of the interstellar medium. Supernova remnants, molecular clouds, and Aurora emission in the geomagnetic pole regions are specific targets for pointing observation. Although the whole system was calibrated before launch, it is essential to perform on-orbit calibration for data analysis. For spectral calibration, we observed airglow lines in the atmosphere since they provide good spectral references. We identify and compare the observed airglow lines with model calculations, and correct the spectral distortion appeared in the detector system to improve the spectral resolution of the system.

• The Journal of the Institute of Internet, Broadcasting and Communication
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• v.10 no.1
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• pp.7-13
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• 2010

We have investigated effects of the rapid thermal annealing of GaN epilayers by molecular beam epitaxy in nitrogen atmosphere. The improvement of structural properties of the samples was observed after rapid thermal annealing under optimum conditions. This improvement in crystal quality is due to a reduction of the spread in the lattice parameter in epilayers. The annealing has been performed in a rapid thermal annealing furnace at $950^{\circ}C$. The effect of rapid thermal annealing on the structural properties of GaN was studied by x-ray diffraction. The Bragg peak shifts toward larger angle as the annealing time increases. As the thermal treatment time increases, FWHM(full width at half maximum) of the peak slightly increase with its decreases followed and it increases again. Results demonstrate that rapid thermal annealing did not always promote qualities of GaN epilayers. However, rapid thermal annealing under optimum conditions improve structural properties of the samples, elevating their crystal quality with a reduction of inaccuracy in the lattice parameter of the epilayers.

• Korean Journal of Crystallography
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• v.18 no.1_2
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• pp.1-6
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• 2007

An Organometallic compound, $C_{16}H_{35}B_{10}IrS_2Si$, was synthesized from o-carborane, $Cp^*Ir(S_2C_2B{10}H_{10})$, and $Me_3SiCHN_2$. The molecular structure of this complex has been determined by X-ray diffraction. Crystallographic data : monoclinic, space group $P2_1/n$, $a=10.1986(12)\;{\AA}$, $b=14.834(5)\;{\AA}$, $c=17.139\;{\AA}$, ${\beta}=92.24(2)^{\circ}$, Z=4, $V=2591.0(14)\;{\AA}^3$. The structure was solved by direct methods and refined by full-matrix leat-squares methods to give a model with a reliability factor R=0.053 for 5080 reflections.

• The Journal of Korean Institute of Electromagnetic Engineering and Science
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• v.12 no.6
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• pp.1009-1017
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• 2001

The acousto-optical spectrometer is designed by using 1 GHz bandwidth acousto-optic deflector for radio signal analysis. This system is a high resolution wide band spectrometer which uses I GHz bandwidth and a total of 2,048 channel charge coupled device. When we measured the spectrums of signals deflected by acousto-optical spectrometer, we confirmed the stability of the total system by repetitive observations of the same frequency, and each part of the system worked well. We installed this system onto 60 cm radio telescope, and observed 12CO(J= 1 ∼0) emission lines around CRL 2688, IRC 10216 and NGC 5005 Galaxy center. We could observe effectively very narrow band width radio spectrum as well as wide band radio spectrum. We also confirmed high sensitivity and resolution in observation of 12CO(J-10) omission line of NGC 5005 Galaxy center which is a weak signal.

• Polymer(Korea)
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• v.25 no.5
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• pp.671-678
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• 2001

Sodium and zinc salts of poly(ethyaene-co-methacrylic acid) ionomers consist of three phases, i.e. ionic aggregates, amorphous, and crystalline phases. Dye molecules after soaked from the methanol solution are located near the amorphous phase or ionic aggregates within ionomer films. Depending on the location of the molecules in the ionomer film, they are under influence of dispersion forces (ethylene parts), polar forces (acid parts). and ionic dipole (ionic aggregates) interactions. The UV/Vis absorption peak of Nile Red under the dispersion force is found at near 500 nm, for the dye under the polar force effect 525 nm, and 550 and 610 nm for the dyes under $Na^+$ and $Zn^{2+}$ ionization effects, respectively. Since the divalent $Zn^{2+}$ ion has larger ionic dipole than the monovalent $Na^+$ ion, the larger red-shift of the absorption band due to the ionic dipole interaction is observed for $Zn^{2+}$ counter ion.

• Proceedings of the Korean Vacuum Society Conference
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• 2013.02a
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• pp.340-341
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• 2013

양자점(Quantum dots; QDs)은 단전자 트랜지스터, 레이저, 발광다이오드, 적외선 검출기와 같은 고효율 광전소자 응용을 위해 활발한 연구가 진행되고 있다. II-VI 족 화합물 반도체는 III-V 족 화합물 반도체와 비교했을 때 더 큰 엑시톤 결합에너지(exciton binding energy)를 가지는 우수한 특성을 보이고 있으며 이러한 성질을 가지는 II-VI 족 화합물 반도체 중에서도 넓은 에너지 갭을 가지는 CdTe 양자점은 녹색 영역대의 광전자 소자로서 활용되고 있다. 기존의 CdTe/ZnTe 양자점을 성장하기 위해 ZnTe와 격자부정합이 적은 GaAs 기판을 이용한 연구가 주를 이룬 반면 Si기판을 이용한 연구는 미흡하다. 하지만 Si 기판은 GaAs 기판에 비해 값이 싸고, 여러 분야에 응용이 가능하며 대량생산이 가능하다는 이점을 가지고 있어 초고속, 초고효율 반도체 광전소자의 제작을 가능케 할 것으로 기대된다. 또한 양자점의 고효율 광전소자에 응용을 위해서는 Si 기판 위에 양자점의 크기를 효율적으로 조절하는 연구 뿐 아니라 양자점의 크기에 따른 운반자 동역학에 대한 연구도 중요하다. 본 연구에선 분자선 에피 성장법(Molecular Beam Epitaxy; MBE)과 원자층 교대 성장법(Atomic Layer Epitaxy; ALE)을 이용하여 Si 기판 위에 성장한 CdTe/ZnTe 양자점의 크기에 따른 광학적 특성을 연구하였다. 저온 광 루미네센스(PhotoLuminescence; PL) 측정 결과 양자점의 크기가 증가함에 따라 더 낮은 에너지영역으로 피크가 이동하는 것을 확인하였다. 그리고 온도 의존 광루미네센스 측정 결과 양자점의 크기가 증가함에 따라 열적 활성화 에너지가 증가하는 것을 관찰하였는데, 이는 양자점의 운반자 구속효과가 증가하였기 때문이다. 또한 시분해 광루미네센스 측정 결과 CdTe/ZnTe 양자점의 크기가 증가함에 따라 소멸 시간이 긴 값을 갖는 것을 관찰하였는데, 이는 양자점의 크기가 증가함에 따라 엑시톤 진동 세기가 감소하였기 때문이다. 이와 같은 결과 Si 기판 위에 성장한 CdTe/ZnTe 양자점의 크기에 따른 열적 활성화 에너지와 운반자 동역학에 대해 이해 할 수 있었다.

• Journal of the Korean Vacuum Society
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• v.9 no.2
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• pp.130-135
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• 2000

We have analyzed characteristics for the structure of $Al_{0.25}/Ga_{0.75}/As/In_{0.15}/Ga_{0.85}$/AS/GaAS pseudomorphic high electron mobility transistor (PHEMT) by photoluminescence (PL) and photoreflectance (PR) measurements. By the PL measurement at 10 K, we observed el-hl transition peak at 1.322 eV and e2-hl transition peak at 1.397 eV in the InGaAs quantum well. We calculated value of 23 meV, the difference between the first energy level and the second energy level of a valence band by dependence of temperatures. Also, (e2-h2) transition signal was observed at 300 K by PR measurement. From the PR measurement, we recognized that the transition was dominated the second energy level of conduction band than the first energy level of conduction band due to band filling. The other hand, PL signal of the first energy level of conduction band was dominated because of the electron screening effect.