• 한국세라믹학회지
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• 제25권4호
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• pp.390-398
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• 1988

Effects of atmospheres and adidtives on the grain growth of TiO2 ceramics were investigated. In the range of 1300~140$0^{\circ}C$, grain growth was increased in CO2 as compared with O2 atmosphere and the grain boundary migration activation energy was lower than the diffusion activation energy of oxygen ion in TiO2. Also, in the case of addition of oxides, the grain growth was increased by oxides acting as a acceptor andinhibited by oxides acting as a donor. From the above results, when the oxygen vacancy concentration was increased, the intrinsic grain boundary mobility was increased and the pore drag force was decreased due to the rapid densification. Also it seems that the pore was migrated by the surface diffusion rather than lattice diffusion.

• 대한기계학회논문집
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• 제6권2호
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• pp.113-120
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• 1982

In the previously reported Part I, the experimental results in frictional machining that finished medium carbon steel SM 50 C under 6 kinds of liquid atmospheres by using ceramic tip as a frictional tool was described. The present study reports the experimental results that all the machining conditions are same in the Part I except tool material changed ceramics into tungsten carbide. The ceramic tool material is a stable oxide and a non-metallic material, but the tungsten carbide has the metallic characteristics that adhere to carbon steel at about 750.deg.C. The present study shows th comparison of the experimental results for the above 2 kinds of frictional tool material.

• 공업화학
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• 제2권3호
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• pp.193-198
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• 1991

후막 구리도체는 귀금속계 도체에 비하여 가격이 저렴하고 전기전도도, 납땜성, 땜납 침식저항, 와이어 본딩성등의 양호한 성질 때문에 매우 중요성을 갖는다. 그러나 우수한 후막 구리도체를 형성하는 것은 구리가 높은 온도에서 쉽게 산화하는 성질로 인해 상당히 복잡하다. 양호한 구리후막을 얻기 위하여 하이브리드 마이크로회로업계는 질소분위기, 반응성분위기 또는 공기분위기를 사용한다. 이 글에서는 후막 구리도체의 소성공정과 세종류의 소성분위기에 대하여 종합적으로 고찰하였다.

• 한국우주과학회:학술대회논문집(한국우주과학회보)
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• 한국우주과학회 2008년도 한국우주과학회보 제17권2호
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• pp.22.3-22.3
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• 2008

We present the results of the investigations of high dispersion spectra of two stars. These are the eclipsing binary RR Lyn, and $\rho$ Pup - the prototype of the group of pulsating variables. The spectra were obtained at 1.8 m Bohyuunsan observatory telescope, and 8.2 m VLT. We found the chemical composition. The both components of RR Lyn are Am stars (metallic line stars), but the abundance patterns of the components are not similar - the iron abundance and the abundances of other elements are surely different. For few elements the differences exceeds 1 dex. We found the abundances of 56 chemical elements in the atmosphere of $\rho$ Pup. This is one of the best stellar abundance patterns. It permits to investigate the role of the charge-exchange reactions in stellar atmospheres. These reactions can produce the abundance anomalies in the atmospheres of B-F type stars. These reactions can be one of the sources of galactic cosmic rays, and the reason of the braked rotation of A-F type chemically peculiar stars.

• 한국전기전자재료학회논문지
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• 제19권2호
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• pp.109-115
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• 2006

Indium tin oxide (ITO) films have been prepared by DC magnetron sputtering. In order to improve the utilization efficiency of the target and reduce the cost of the film deposition processes, the powder target was used instead of the conventional ceramic target. As-deposited films were annealed at temperatures between $200^{\circ}C$ and $500^{\circ}C$ for 30 min in air. Also, the film was annealed in various atmospheres such as air, $O_2,\;H_2,\;N_2$, and vacuum at $400^{\circ}C$C for 30 min. Effects of the heat treatment conditions on structural, electrical, and optical properties of ITO films were investigated. The annealing temperature of $400^{\circ}C$ and atmospheres of $H_2$ and $N_2$ seem to be the most suitable conditions for post processing.

• Journal of Electrochemical Science and Technology
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• 제4권4호
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• pp.153-156
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• 2013

Charge transfer between STM tip and Au(100) has been investigated by using a Scanning Tunneling Microscopy (STM) technique in dry, $H_2O$, and $D_2O$ atmospheres. Dry atmosphere was indicated by humidity as low as 5 % and high humidity as high as 98% was managed by injecting $H_2O$ and $D_2O$ to the chamber. The current decayed more slowly in high humidity than in dry atmosphere. The plateau currents were found to appear at separations larger than ca. $5{\AA}$ where the current decay stopped depending on applied bias voltages. The polarity dependence was observed at the STM junction between Pt-Ir tip and the gold. On the contrary, little dependence was seen at the one between Au tip and the substrate electrode.

• 한국세라믹학회지
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• 제36권11호
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• pp.1198-1204
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• 1999

The effect of sintering atmosphere on the grain sizes and phase distributions in 3Y-ZrO2 and 8Y-ZrO2 was investigated O2 and N2 were used as sintering atmospheres. In the case of 3Y-ZrO2 the sintered density was higher in N2 than in O2 while in the case of 8Y-ZrO2 contrary results were obtained. The observation can be explained by the nitrogen solubility into the zirconia lattice. That is nitrogen gas can behave as a diffusive gas contrary to the behavior in other oxides depending on the amount of Y2O3. In 3Y-ZrO2 tetragonal phase was retained at room temperature irrespective of sintering atmospheres. Grain sizes of two specimens were below 2㎛ and larger in O2 thin in N2 Under a given stress the transformability of tetragonal phase into monoclinic phase was higher in O2 than N2. The results are discussed on the basis of an effect of the grain size and non-transformable ttragonal(t') phase.

• Journal of international Conference on Electrical Machines and Systems
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• 제1권1호
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• pp.128-134
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• 2012

This paper gives an overview of the requirements for electrical equipment in potentially explosive atmospheres and describes how these are applied to electrical machines and drives in hazardous areas. The method by which equipment can be shown to be safe in a whole range of gases, by testing in a single test gas, is covered. It is shown how the more recently introduced methods of protection for hazardous areas, increased safety and nonsparking, are ideally suited to AC machines and drives. A novel method of measuring the fullload temperature rise of electrical machines for hazardous, and other areas, without the need to connect a mechanical load to the machine's drive shaft is explained.

• 천문학논총
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• 제30권2호
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• pp.423-427
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• 2015

Recognition of the role of radio galaxies in the universe has been increasing in recent years. Their colossal energy output over huge volumes is now widely believed to play a key role not only in the formation of galaxies and their supermassive black holes, but also in the evolution of clusters of galaxies and, possibly, the cosmic web itself. In this regard, we need to understand the inflation of radio bubbles in the hot gas atmospheres of clusters and the importance of the role that radio galaxies play in the overall energy budget of the intracluster medium. Here, we present results from X-ray and radio band observations of the hot gas atmospheres of powerful, nearby radio galaxies in poor clusters.

• 한국재료학회지
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• 제3권6호
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• pp.575-584
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• 1993

주조용 Ni기 초내열 합금인 Rene 80의 고온 크리프타단시 균열의 생성과 전파에 대한 분위기의 영향을 조사하기 위해 $760^{\circ}C$, 675MPa및 $982^{\circ}C$, 157MPa의 크리프시험 조건에서 산화성 분위기인 공기중과 불활성 분위기인 아르곤 가스 분위기에서 크리프 파단시험을 했다. $760^{\circ}C$, 657MPa조건의 크리프 파단시험에서는 분위기에 따라 크리프 파단 양상의 큰 차이가 없었고 파단수명과 파단연신값도 비슷하였다. 반면 $982^{\circ}C$, 157MPa의 시험에서는표면산화의 영향으로 공기중의 경우 표면균열 생성과 입계를 통한 균열전파에 의하여 크리프 파단이 진행되었으나, 아르곤 분위기에서는 내부입계에서 균열이 생성되어 표면에서 발생된 균열과 합체됨으로서 파단이 진행되었다. 파단수명은 공기중의 경우가 치밀한 표면산화물의 형성에 따라 아르곤 하에서 보다 길었으며 파단연신은 아르곤 분위기의 경우가 네킹 발생에 따라 크게 나타났다.