• 한국반도체및디스플레이장비학회:학술대회논문집
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• 한국반도체및디스플레이장비학회 2005년도 추계 학술대회
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• pp.35-39
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• 2005

Phosphor powders of zinc gal late added with Mg and rare-earth elements were prepared by sol id state reaction to improve luminescent properties. Green emitting $ZnMnGa_{2}O_{4}$ reached maximum intensity at Mn=0,005 mole$\%$ and further improvement was achieved by addition of $Mg^{2+}$. Tm, Mg-added zinc gallate phosphor exhibited a strong blue band emission, peaking at about 420 nm with the maximum intensity at the concentration of 0.003 mole$\%$ Mg and 0.015 mole$\%$ Tm. Deepening of the potential wells of the ground and excited states was suggested to be the cause for the enhancement in emission intensity at optimal doping of Mg and Tm.

• 한국전기전자재료학회:학술대회논문집
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• 한국전기전자재료학회 2009년도 하계학술대회 논문집
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• pp.277-278
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• 2009

We have studied an angular dependence of emission pattern of top-emssion organic light-emitting diodes (TEOLED). Device structure is Al(100nm)/TPD(40nm)/$Alq_3$(60nm)/LiF(0.5nm)/Al(2nm)/Ag(30nm). N,N'-diphenyl-N,N'-di(m-tolyl)-benzidine (TPD) and tris-(8-hydroxyquinoline) aluminium ($Alq_3$)were used as a hole transport layer and emission layer, respectively. Organic layers and cathode were thermally evaporated at $2\times10^{-5}$torr. The evaporation rate of the organic material was maintained to be $1.5\sim2.0{\AA}/s$, and that of metal layer to be $0.5\sim5{\AA}/s$. A transmittance of a cathode electrode(Al/Ag) in visible region is about 25~30%. In order to measure view-angle dependent intensity, electroluminenscence spectra of the device at each angle were integrated. Angle dependent emission spectra of the device do not show blue shift. Emission intensity of the device that the going straight characteristic is stronger the bottom-emission organic light-emitting diodes is shown.

• 천문학회보
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• 제36권1호
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• pp.88.2-88.2
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• 2011

The far-ultraviolet (FUV) continuum and spectral images of C IV and H2 emission lines for the region of Orion-Eridanus Superbubble (OES) are hereby presented and compared with the maps obtained in other wavelengths. While the region shows complex structures, consisting of hot gases and cold dust, a close examination reveals that the FUV emission in this region can be understood reasonably as the result of their interactions. We confirm the origin of most diffuse FUV continuum to be starlight scattered by dust, but we also find that the ionized gas also contributes 50-70% of the total FUV intensity in the regions of H_alpha arcs. We note the bright diffuse FUV continuum in the eastern part of the northern dust-rich region, and attribute it to the bright early-type stars more abundant in this region than in the west as the amount of dust itself does not seem to be much different across 'arc A' that separates the two regions. In addition, two P Cygni-type stars are identified in this eastern region and their peculiar spectral profiles around the C IV emission line are anifested in the scattered diffuse spectrum. Besides this, the C IV emission is generally enhanced at the boundaries of the hot X-ray cavities where thin dust regions are located, confirming the thermal interface nature of the origin of this cooling emission line. The morphology of the H2 emission shows a general correlation with dust extinction features but its intensity peaks are rather located in thin dust areas, off the peak dust regions. Furthermore, H2 emission is seen to be weak in the arc A region though the arc passes through the center of the dust-rich area. Hence, the H2 emission and dust features, together with those of X-ray and ion lines emissions, show stratified structure of arc A quite well, again confirming its thermal interface nature.

• 자원ㆍ환경경제연구
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• 제15권3호
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• pp.425-450
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• 2006

산업부문은 생산 활동을 담당하는 특성 때문에 많은 에너지를 소비하고 많은 $CO_2$를 배출한다. 산업부문 중에서 에너지다소비산업이라고 일컬어지는 산업들은 다른 산업에 비해서 에너지소비가 많고 $CO_2$ 배출을 많이 하므로 관련정책의 목표대상으로서 우선적으로 거론된다. 그러나 해당 산업의 생산액과 $CO_2$ 배출량을 사용하는 환경원단위는 해당 산업만의 환경오염물질 배출의 정도를 측정하기에는 적합하지만, 산업들이 유기적으로 연결되어 서로 생산품을 수요하고 공급하고 있는 점을 고려한다면 환경원단위를 확대시킨, 그리고 산업 전체를 고려하는 지표로 해당 산업의 환경물질의 배출 정도를 평가해야 한다. 이에 본 논문에서는 우리나라의 환경산업연관표 2000을 작성하고, 에너지다소비산업 외에 전 산업을 대상으로 하여 산출액기준 및 열량기준의 환경원단위와, 이를 보다 확대하고 산업의 유기적 관계까지를 모두 고려하는 유발 $CO_2$ 발생량을 추정하여 우리나라의 경제주체간 및 산업간의 상품생산과 흐름에 수반되는 에너지소비와 환경오염물질의 흐름을 분석하였다. 분석결과에 따르면 산출액기준 및 열량기준의 환경원단위가 상대적으로 높은 산업들의 유발 $CO_2$ 발생량은 크다. 이 산업들은 직접적으로 발생시키는 $CO_2$가 많은 산업들이며, 환경부하가 큰 재화나 서비스를 생산한다. 그러므로 이 산업들을 대상으로 환경원단위 저감을 유도한다면 $CO_2$ 발생량을 감소시킬 수 있다. 그러나 환경원단위가 낮은 산업의 생산 시에 환경원단위가 높은 산업들의 생산품이 투입재로 사용된다면 그 산업의 유발 $CO_2$ 발생량은 커지고 경제 전체의 환경부하를 크게 만든다. 따라서 산출액기준의 환경원단위가 높은 산업들만을 중심으로 하여 환경원단위를 저하시키는 것 외에, 낮은 환경원단위를 갖는 산업들의 환경원단위도 지속적으로 감소시켜 다른 산업에 대한 연관을 통한 유발 $CO_2$ 발생량을 감소시켜야 한다. 이는 모든 산업에 대한 지속적인 환경원단위 저감이 경제 전체를 기준으로 더 큰 $CO_2$ 발생량 저감을 유도하는 것을 의미한다.

• Bulletin of the Korean Chemical Society
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• 제29권7호
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• pp.1353-1358
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• 2008

Benzyl arylether dendrimers with zinc porphyrin core and terminal vinyl groups have been synthesized and their photophysical properties and the influence of dendritic environments were investigated. Free base porphyrin-cored benzyl arylether dendrimers 1a-1c and 3a-3c, and their zinc derivatives 2a-2c and 4a-4c have been prepared. Absorption spectra are similar for all porphyrin-cored benzyl arylether dendrimers, except that absorption intensity at 280 nm increases in the higher generation of dendrimer. Fluorescence spectra are similar with two bands for all free base porphyrin dendrimers 1a-1c and 3a-3c, although fluorescence intensity ratio of shorter wavelength emission band to longer wavelength band varies with the generation of dendrimer. Emission efficiencies of 1a-1c and 3a-3c are lower than that of TTP. Emission efficiencies of 2a-2c and 4a-4c are higher than that of ZnTTP. Absorption and emission properties of 1a-1c, 2a-2c, 3a-3c, and 4a-4c were affected negligibly with dendritic environments.

• 한국재료학회지
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• 제11권9호
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• pp.740-744
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• 2001

The $Y_2SiO_5:Ce$ phosphors were synthesized by sol-gel technique in order to improve the performance of blue emitting phosphors for field emission display(FED). The resulted$Y_2SiO_5:Ce$ phosphors enhanced the emission intensity. In addition, calcination temperature of sol-gel technique(1300~140$0^{\circ}C$) was lower than that of the solid state reaction(>1$600^{\circ}C$). Under 365 nm and low voltage electron excitations. $Ce^{3+}$ -activated $Y_2SiO_5$phosphors showed blue emission band with a range of 400~ 430nm. Especially, 2mol% $Ce^{3+}$ doped $Y_2SiO_5:Ce$phosphors showed the maximum emission intensity. We have also controlled drying temperature of wet gel, pH, and $H_2O$/TEOS molar ratio for the optimum condition of TEOS hydrolysis.

• 한국진공학회지
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• 제15권5호
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• pp.541-546
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• 2006

본 연구에서는 박막형 $ZnGa_2O_4:Mn$ 산화물 형광체의 음극선루미느센스 특성과 구조적 성질에 대하여 field emission scanning electron microscopy (FESEM), atomic force microscopy (AFM), photoluminescence (PL), 그리고 cathodoluminescence (CL) 방법을 이용하여 조사하였다. $ZnGa_2O_4:Mn$ 형광체 타겟으로부터 $Mn^{2+}$ 이온의 $^4T_1{\rightarrow}^6A_1$ 전이에 의한 506nm 파장에서의 PL emission 스펙트럼이 관찰되었다. 색좌표는 x = 0.09, y = 0.67 이었다. $ZnGa_2O_4:Mn$ 박막의 여기 스펙트럼은 $Mn^{2+}$ 이온 흡수에 의한 294 nm의 피크 파장을 나타내었다. 낮은 압력에서 증착한 $ZnGa_2O_4:Mn$ 형광체 박막은 고밀도의 치밀한 단면구조를 보였고, 높은 세기의 음극선루미느센스가 505 nm 피크 파장에서 나타났다. 표면 거칠기가 음극선루미느센스의 세기에 미치는 영향은 관찰되지 않았다.

• 천문학회지
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• 제29권spc1호
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• pp.171-172
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• 1996

We present the results of an rocket-borne observation of far-infrared [CII] line at 157.7 ${\mu}m$ from the diffuse inter-stellar medium in the Ursa Major. We also introduce a part of results on the [CII] emission recently obtained by the IRTS, a liquid-helium cooled 15cm telescope onboard the Space Flyer Unit. From the rocket-borne observation we obtained the cooling rate of the diffuse HI gas due to the [CII] line emission, which is $1.3{\pm}0.2 {\times} 10^{-26}$ $ergss^{-1} H^{-1}_{atom}$. We also observed appreciable [CII] emission from the molecular clouds, with average CII/CO intensity ratio of 420. The IRTS observation provided the [CII] line emission distribution over large area of the sky along great circles crossing the Galactic plane at I = $50^{\circ}$ and I = $230^{\circ}$. We found two components in their intensity distributions, one concentrates on the Galactic plane and the another extends over at least $20^{\circ}$ in Galactic latitude. We ascribe one component to the emission from the Galactic disk, and the another one to the emission from the local interstellar gas. The [CII] cooling rate of the latter component is $5.6 {\pm} 2.2 {\times}10$.

• 한국재료학회지
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• 제15권6호
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• pp.419-425
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• 2005

In this paper, we describe the luminescent properties of the phosphors synthesized via sol-gel technique. When the phosphor prepared by sol-gel technique, reaction factors, such as pH condition, $R_w$ and drying temperature affected the luminescent intensity, particle size and morphology of final product. Therefore, we attempt to control these reaction factors in order to improve the luminescent efficiency of phosphors. As a result of our study, when the acid catalyst (HCl) was used, emission intensity was higher than the case of base catalyst $(NH_4OH)$. The product prepared at $R_w=60$ indicated the maximum intensity. As the increase of the $R_w$ value, the particle was agglomerated and emission intensity was decreased. Finally, optimum drying temperature of gel was found to be$ 180^{\circ}C$.

• 천문학회지
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• 제50권4호
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• pp.105-109
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• 2017

The well-known solar cycle controls almost the entire appearance of the solar photosphere. We therefore presume that the continuous emission of visible light from the solar surface follows the solar cyclic variation. In this study, we examine the solar cyclic variation of photospheric brightness in the visible range using solar images taken by the Solar and Heliospheric Observatory (SOHO)/Michelson Doppler Imager (MDI). The photospheric brightness in the visible range is quantified via the relative intensity acquired from in the raw solar images. In contrast to total solar irradiance, the relative intensity is out of phase with the solar cycle. During the solar minimum of solar cycles 23-24, the relative intensity shows enhanced heliolatitudinal asymmetry due to a positive asymmetry of the sunspot number. This result can be explained by the strength of the solar magnetic field that controls the strength of convection, implying that the emission in the visible range is controlled by the strength of convection. This agrees with the photospheric brightness increasing during a period of long spotless days.