• 방사선산업학회지
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• 제8권1호
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• pp.59-63
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• 2014

Proton Induced X-ray Emission (PIXE) is a MeV ion beam analysis method for use with particle accelerators. PIXE uses low-energy charged particles as an excitation mechanism to generate characteristic x-ray emission from each element in a target. In PIXE analysis, the beam current used is from a few nA to several tens of nA. Chosun University (Cyclotron Research Center) designed a $50{\mu}A$ beam line from the 13 MeV cyclotron for use with a PIXE analysis system, as well as performing beam transport line optimization research. In this study, the beam line operation conditions for the optimization process of beam transport and beam characteristics are shown.

• 한국표면공학회:학술대회논문집
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• 한국표면공학회 2014년도 추계학술대회 논문집
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• pp.185-185
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• 2014

In this study, we investigated surface characteristics of hydroxyapatite coated surface on nano/micro pore structured Ti-35Ta-xNb alloys. This paper was focus on morphology and corrosion resistance of Anodic oxidation. To prepare the samples, Ti-35Ta-xNb (x= 0, 10 wt. %) alloys were manufactured by arc melting and heat-treated for 12 h at $1050^{\circ}C$ in Ar atmosphere at $0^{\circ}C$ water quenching. Micro-pore structured surface was performed using anodization with a DC power supply at 280 V for 3 min, nanotube formed on Ti-35Ta-xNb alloys was performed using DC power supply at 30 V in 60 min at room temperature. Surface morphology and structure were examined by field-emission scanning electron microscopy, energy-dispersive X-ray spectroscopy and X-ray diffraction.

• 한국세라믹학회지
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• 제38권9호
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• pp.817-821
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• 2001

새로운 형광체로 역스피넬 구조를 갖는 $Mg_{2-x}MN_xSnO_4$ 조성을 선정하여 고상반응에 의하여 제조하였다. $Mg_2SnO_4:Mn$의 광발광 특성이 147nm 파장의 진공 자외선 여기하에 측정되었다. Mn의 첨가에 의하여 $Mg_2SnO_4$ 형광체는 500nm 파장에 발광 중심을 가지며 매우 높은 발광강도를 나타내었다. 이것은 스피넬 구조의 산소 사면체 배위에 위치하는 Mg 자리를 치환하여 들어가는 $Mn^{2+}$ 이온의 $^4T_1$ 상태로부터 $^6A_1$ 상태로의 에너지 전이에 의한 발광으로 해석되었다. 진공 자외선 여기하에 최대의 발광강도를 나타내는 Mn 활성제의 농도는 0.25mol%이었고, 잔광시간은 10ms 이하인 것으로 조사되었다.

• 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.

• 천문학회보
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• 제37권2호
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• pp.99.2-99.2
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• 2012

We updated the far-ultraviolet (FUV) spectral images of the entire Vela supernova remnant (SNR) using newly processed FIMS/SPEAR data. In the present study, we compare the newly produced FUV images with the X-ray and $H{\alpha}$ images, and examine how the Vela SNR evolves and interacts with the ambient medium on a global scale. The comparison with X-ray images has revealed a FUV filamentary feature corresponding with the boundary of the northeast-southwest asymmetry of the X-ray shell. The relatively low O IV] ${\lambda}1404$ to O III] ${\lambda}{\lambda}1661$, 1666 ratio estimated on the FUV filament is compatible with the previous proposal that the observed asymmetry of the Vela SNR could be due to the ${\gamma}2$ Velorum stellar wind bubble (SWB). The southwest FUV features surrounding a faint extended X-ray region are characterized as the region where the Vela SNR is interacting slightly stronger with ambient mediums within the dim X-ray southwest section. From a comparison with the $H{\alpha}$ image, we identify a ring-like $H{\alpha}$ feature overlapped with an extended hot X-ray feature of similar size and two local peaks of C IV ${\lambda}{\lambda}1548$, 1551 emission. Their morphologies are consistent with the expected shape when the $H{\alpha}$ ring is in direct contact with the near or far side of the Vela SNR. We suggest that the B3V-type star HD 76161 found at the center of the $H{\alpha}$ ring would be the exciting source of the H II region.

• 한국우주과학회:학술대회논문집(한국우주과학회보)
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• 한국우주과학회 2000년도 한국우주과학회보 제9권1호
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• pp.24-24
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• 2000

No Abstract, See Full Text

• 한국진공학회:학술대회논문집
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• 한국진공학회 2009년도 제37회 하계학술대회 초록집
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• pp.171-171
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• 2009

• 한국정보통신학회:학술대회논문집
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• 한국해양정보통신학회 2008년도 추계종합학술대회 B
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• pp.95-99
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• 2008

반도체 소자의 소형화에 따라 낮은 비저항을 가진 구리가 ULSI의 금속배선으로 사용되고 있다. 구리선의 비저항은 RC delay와 집적회로의 신호전달에 영향을 미치게 된다. 본 논문에서는 전기도금 된 구리박막의 비저항에 대해 전해액이 미치는 영향을 조사하였다. 4탐침 표면저항측정기로 비저항을 평가하였고, XRD (X-ray Diffraction), AFM (Atomic Force Microscope), FE-SEM (Field Emission Scanning Electron Microscope), XPS (X-ray Photoelectron Spectroscopy)로 박막의 특성을 조사하였다. 실험한 결과, 전해액의 조건이 전기도금으로 증착된 낮은 비저항을 갖는 구리박막의 형성에 있어 중요한 역할을 하는 것을 확인하였다.

• 공업화학
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• 제20권6호
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• pp.617-621
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• 2009

Zinc oxide (ZnO)을 금(Au)과 fluorine-doped tin oxide (FTO) 촉매로 산화실리콘($SiO_2$) 기판에 산화아연입자 20 nm, $20{\mu}m$를 각각 사용하여 기체-액체-고체(VLS) 합성법으로 성장시켰다. 나노로드의 표면특성, 화학조성, 그리고 결정특성을 엑스레이회절(X-ray diffraction (XRD)), 에너지 분산형 X선 분광기(Energy-dispersive X-ray spectroscopy (EDX)), 표면 방출주사현미경(Field-emission scanning electron microscope (FE-SEM))으로 분석하였다. ZnO의 입자 크기 뿐만 아니라 결정형태가 성장에 크게 영향을 미쳤다. ZnO의 모든 나노구조가 6방정계(六方晶系), 단일결정구조를 가지고 있었다. 최적온도는 $1030^{\circ}C$, 입자크기는 20 nm이다. 그러므로 Au 대신 플루오린 첨가 도핑으로 전기음성도가 증가된 FTO 증착에 의해서 생성된 나노로드는 경제성 있는 대체물질로서의 가치가 있을 것으로 사료된다.

• 한국재료학회지
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• 제4권5호
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• pp.510-515
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• 1994

플라즈마 화학 증착법으로 (100)p-type Si wafer위에 $Y_2O_3$-Stabilzed $ZrO_2$박막을 증착하였다. 반응 기체로는 zirconium triflouracethylacetonate[Zr(tfacac) $[Zr(tfacac)_4]$, tri(2.2.6.6 tetramethy1-3, 5-heptanate) yttrium $[Y(DPM)_3]$과 oxygen gas를 사용하였다. X-ray diffraction(XRD)과 fourier Particle induced x-ray emission(PIXE)을 통하여 $Y(DPM)_3$ bubbling temperature가 $160^{\circ}C, 165^{\circ}C, 170^{\circ}C$일때 $Y_2O_3$함량이 12.1mo1%, 20.4mol%, 31.6mol%임을 알 수 있었다. C-V측정에서 $Y(DPM)_3$ bubbling temperature가 증가함에 따라 flat band voltage가 더욱더 음의 방향으로 이동하였다.