• 한국수소및신에너지학회논문집
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• 제24권1호
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• pp.29-35
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• 2013

A dense mixed ionic and electronic conducting ceramic membrane is one of the most promising materials because it can be used for separation of oxygen from the mixture gas. The $ABO_3$ perovskite structure shows high chemical stability at high temperatures under reduction and oxidation atmospheres. $BaCo_{1-x-y}Fe_xZr_yO_{3-{\delta}}$ (BCFZ) was well-known material as high mechanical strength, low thermal conductivity and stability in the high valence state. Glycine Nitrate Process (GNP) is rapid and effective method for powder synthesis using glycine as a fuel and show higher product crystallinity compared to solid state reaction and citrate-EDTA method. BCFZ was fabricated by modified glycine nitrate process. In order to control the burn-up reaction, $NH_4NO_3$ was used as extra nitrate. According to X-Ray Diffraction (XRD) results, BCFZ was single phase regardless of Zr dopants from y=0.1 to 0.3 on B sites. The green compacts were sintered at $1200^{\circ}C$ for 2 hours. Oxygen permeability, methane partial oxidation rate and hydrogen production ability of the membranes were characterized by using Micro Gas Chromatography (Micro GC) under various condition. The high oxygen permeation flux of BCFZ 1-451 was about $1ml{\cdot}cm^{-2}s^{-1}$. Using the humidified Argon gas, BCFZ 1-433 produced hydrogen about $1ml{\cdot}cm^{-2}s^{-1}$.

• 한국분말재료학회지
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• 제15권3호
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• pp.182-187
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• 2008

Carbon was known to be one of effective additives which can improve the flux pinning of $MgB_2$ at high magnetic fields. In this study, glycerin $(C_3H_8O_3)$ was selected as a chemical carbon source for the improvement of critical current density of $MgB_2$. In order to replace some of boron atoms by carbon atoms, the boron powder was heat-treated with liquid glycerin. The glycerin-treated boron powder was mixed with an appropriate amount of magnesium powder to $MgB_2$ composition and the powder pallets were heat treated at $650^{\circ}C\;and\;900^{\circ}C$ for 30 min in a flowing argon gas. It was found that the superconducting transition temperature $(T_c)$ of $Mg(B_{1-x}C_x)_2$ prepared using glycerin-treated boron powder was 36.6 K, which is slightly smaller than $T_c$(37.1 K) of undoped $MgB_2$. The critical current density $(J_c)$ of $Mg(B_{1-x}C_x)_2$ was higher than that of undoped $MgB_2$ and the $T_c$ improvement effect was more remarkable at higher magnetic fields. The $T_c$, decrease and $J_c$ increase associated with the glycerin treatment for boron powder was explained in terms of the carbon substitution to boron site.

• 한국결정학회지
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• 제3권1호
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• pp.37-43
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• 1992

비선형광학 단결정인 KTiOP04는 Nd:YAG 레 이저의 제2고조파 발생장치로 가장 널리 이용되 는 물질이다. 본 연구에서는 낮은 점도를 갖는 3K2W04. P2O5 응제를 이용하여 TSSG법에 의한 KTiOP04 단결 정 육성 실 험 을 하였다. KTiOP04 육 성에 적합하도록 온도구배가 작은 전기로와 정밀 한 회전인상장치를 제작하였으며,용액 내 수직온도 구배는 용액표면과 용액 밑부분의 온도차가 1℃로 매우 작았다. 성장 과정의 관찰과 조절이 용이하도록 종자정을 용액 표면에 위치시켰다. 용액의 조성은 66.7mol%의 KTiOP04를 포함하도록 고정하였으며 이 용액의 포화온도는 1020℃ 였다. 냉각속도가 0 2℃/h, 결정의 회전속도가 50 rpm인 성장조건에서 a-, b-, c-축으로의 길이 가 각각 23 ×25 ×25mm3인 포유물이 없는 양질의 단결정을 얻을 수 있었다. 성장된 K,Tiop04 단결정은 크게 발달한 (201)면과 (011), (110), (100) 면들로 이루어져 있었으며 (101) 면이 관찰되기도 하였다.

• 헤리티지:역사와 과학
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• 제55권3호
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• pp.120-129
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• 2022

본 연구는 조선시대 대형 불화 10점에 사용된 회청 안료에 대하여 에너지분산형X-선분광기를 이용하여 화학 조성 분석을 시행하고, 편광현미경과 주사전자현미경을 이용하여 형태적 특성을 관찰하여 재질 및 특성을 밝히고자 한다. 화학 조성 분석에 의하면, 10개의 대형 불화의 회청은 모두 주제로 SiO₂, 융제로 K₂O를 사용한 포타쉬 유리로 판단된다. 착색제로 사용한 코발트 광석과 관련된 성분 외에도 As₂O₃, BaO, PbO가 높게 검출되는 대형 불화가 확인된다. 회청 입자들은 일정한 형태가 없고, 다양한 색도의 청색을 띤다. 일부 입자에서는 패각상의 깨짐, 구 모양의 기포, 불순물이 관찰된다. 반사전자상을 통해 AD 18세기 초반의 대형 불화에서 나온 회청은 As가 높은 회청만 검출되었으나 AD 18세기 중반 이후의 대형 불화에서 나온 회청에서는 입자마다 다양한 명암 차이가 확인되었으며 As, Ba, Pb 등이 높은 회청이 검출된다. 이상의 결과를 통해 조선시대 대형 불화의 회청 유형은 3가지로 구분된다. A형은 As₂O₃가 높은 유형, B형은 BaO가 높은 유형, C형은 PbO가 높은 유형이다. 회청 안료의 3가지 유형을 대형 불화의 제작 시기별로 살펴보면, A형은 중간에 검출되지 않은 시기도 있지만 1705년부터 1808년까지 사용이 확인되며, B형과 C형은 1750년부터 출현하여 1808년까지 사용된 것을 알 수 있다. 이는 AD 18세기 초반까지는 한 가지 유형의 회청만 사용되었고, AD 18세기 중반부터는 하나의 대형 불화 안에서도 여러 유형의 회청이 혼합되어 사용된 것을 알 수 있다. 이와 같은 연구는 당시 대형 불화를 제작할 때 사용한 회청 안료의 특성을 이해할 수 있는 정보를 제공할 것으로 기대된다.

• 대한기계학회논문집B
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• 제21권9호
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• pp.1115-1125
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• 1997

Experiments have been conducted to obtain local and average heat transfer coefficients associated with impingement of a row of circular, free surface-water jets on a constant heat flux surface. Nozzle arrays are a row of 3 jets (nozzle dia.=4.6 mm) and a row of 5 jets (nozzle dia.=3.6 mm), and the nozzle configuration is Reverse cone type revealed good performance in heat transfer. Nozzle-to-plate spacings ranging from 16 mm to 80 mm were investigated for two jet center to center spacings 25 mm and 37.5 mm in the jet velocity of 3 m/s (R $e_{D}$=27000) to 8 m/s (R $e_{D}$=70000). For a row of 3 jets and a row of 5 jets, the stagnation heat transfer of the central jet is lower than that of adjacent jets. In the wall jet region between jets, for small nozzle-to-plate spacing and large jet velocity, the local maximum in the Nusselt number was observed, however, for small jet velocity or large nozzle-to-plate spacing, the local maximum was not observed. Except for the condition of $V_{O}$=8 m/s and H/D=10, the average Nusselt number reveals the following ranking: a row of 5 jets, a row of 3 jets, single jet. For a row of 3 jet, the maximum average Nusselt number occurs at H/D=8 ~ 10, and for a row of 5 jets, it occurs at H/D=2 ~ 4. Compared with the single jet, enhancement of average heat transfer for a row of 3 jets is approximately 1.52 ~ 2.28 times, and 1.69 ~ 3.75 times for a row of 5 jets.ets.s.

• 한국자기학회지
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• 제16권5호
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• pp.255-260
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• 2006

기본조성 $(Ni_{0.35}Cu_{0.2}Zn_{0.45})_{1.02}(Fe_2O_3)_{0.98}$과 NiO 비율을 증가시키고 ZnO을 감소시킨 또 다른 기본조성 $(Ni_{0.4}Cu_{0.2}Zn_{0.4})_{1.02}(Fe_2O_3)_{0.98}$에 grain boundary의 높은 저항층을 형성하고 flux로서 사용하기 위해서 0.1 mol% $CaCO_3$와 입자의 성장을 촉진시켜 낮은 손실, 높은 투자율을 얻기 위한 목적으로 $V_2O_5$를 0.03mo1% 첨가하였다. 이들 원료들을 혼합한 후 $600^{\circ}C$에서 2시간 동안 가소시킨 분말을 toroid 시편으로 만들어 소결온도 $1,050^{\circ}C,\;1,070^{\circ}C,\;1,100^{\circ}C$에서 각각 2시간 동안 공기 중에서 소결하였다. 각 시편들에 대한 밀도는 $4.90{\sim}5.10g/cm^3$으로 나타났고, 각 시편들의 고유저항은 $10^8{\sim}10^{12}{\Omega}-cm$으로 측정되었으며, 결정립의 크기는 대략 $3.0{\sim}8.0{\mu}m$이었다. 시편들의 자기유도 특성 값이 대부분 우수하게 나타났으며, 그 중에서도 기본조성 $(Ni_{0.4}Cu_{0.2}Zn_{0.4})_{1.02}(Fe_2O_3)_{0.98}$에 $CaCO_3$와 $V_2O_5$를 첨가하고 $1,070^{\circ}C$에서 소결한 시편의 특성 값이 잔류자기유도 1,660 G, 최대자기유도 4,000 G로 약간 더 우수하게 측정되었으며, 각각 시편들의 보자력은 $0.15{\sim}0.25\;Oe$로 전형적인 연자성 재료의 범위로 나타났다. 초투자율, 손실계수, 및 큐리온도는 각각 $2,948{\sim}2,997,\;171{\sim}208,\;191{\sim}202^{\circ}C$로 나타나 Ni-Zn ferrite에서 측정되는 값들과 대동소이했다. 물리적인 특성값(고유저항, 자기유도, 초투자율, 손실계수, 큐리온도 등)으로 미루어보아 각종 microwave 통신기기 core 및 고 투자율 deflection yoke core 등으로 사용이 가능하다.

• 한국진공학회:학술대회논문집
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• 한국진공학회 2013년도 제44회 동계 정기학술대회 초록집
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• pp.183-184
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• 2013

Two main MBE growth techniques have been used: plasma-assisted MBE (PA-MBE), which utilizes a rf plasma to supply active nitrogen, and ammonia MBE, in which nitrogen is supplied by pyrolysis of NH3 on the sample surface during growth. PA-MBE is typically performed under metal-rich growth conditions, which results in the formation of gallium droplets on the sample surface and a narrow range of conditions for optimal growth. In contrast, high-quality GaN films can be grown by ammonia MBE under an excess nitrogen flux, which in principle should result in improved device uniformity due to the elimination of droplets and wider range of stable growth conditions. A drawback of ammonia MBE, on the other hand, is a serious memory effect of NH3 condensed on the cryo-panels and the vicinity of heaters, which ruins the control of critical growth stages, i.e. the native oxide desorption and the surface reconstruction, and the accurate control of V/III ratio, especially in the initial stage of seed layer growth. In this paper, we demonstrate that the reliable and reproducible growth of GaN on Si (110) substrates is successfully achieved by combining two MBE growth technologies using rf plasma and ammonia and setting a proper growth protocol. Samples were grown in a MBE system equipped with both a nitrogen rf plasma source (SVT) and an ammonia source. The ammonia gas purity was ＞99.9999% and further purified by using a getter filter. The custom-made injector designed to focus the ammonia flux onto the substrate was used for the gas delivery, while aluminum and gallium were provided via conventional effusion cells. The growth sequence to minimize the residual ammonia and subsequent memory effects is the following: (1) Native oxides are desorbed at $750^{\circ}C$ (Fig. (a) for [$1^-10$] and [001] azimuth) (2) 40 nm thick AlN is first grown using nitrogen rf plasma source at $900^{\circ}C$ nder the optimized condition to maintain the layer by layer growth of AlN buffer layer and slightly Al-rich condition. (Fig. (b)) (3) After switching to ammonia source, GaN growth is initiated with different V/III ratio and temperature conditions. A streaky RHEED pattern with an appearance of a weak ($2{\times}2$) reconstruction characteristic of Ga-polarity is observed all along the growth of subsequent GaN layer under optimized conditions. (Fig. (c)) The structural properties as well as dislocation densities as a function of growth conditions have been investigated using symmetrical and asymmetrical x-ray rocking curves. The electrical characteristics as a function of buffer and GaN layer growth conditions as well as the growth sequence will be also discussed. Figure: (a) RHEED pattern after oxide desorption (b) after 40 nm thick AlN growth using nitrogen rf plasma source and (c) after 600 nm thick GaN growth using ammonia source for (upper) [110] and (lower) [001] azimuth.

• 한국식품저장유통학회지
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• 제22권6호
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• pp.804-810
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• 2015

본 연구에서는 고품질 단삼을 생산하기 위한 재배지대 구분과 수확시기에 따른 단삼의 생산성 및 성분함량에 대한 기초자료를 확보하기 위하여 온도조건별 생리반응과 수확시기별 품질을 조사하였다. 동화산물의 축적과 수분이용 효율에 영향을 미치는 광합성율, 증산율 및 엽록소 형광반응을 조사한 결과 $20^{\circ}C$에서 광합성율, 기공전도도, 수분이용 효율이 가장 좋았고 광보상점이 가장 낮아 약광조건에서도 광합성 효율이 높았으며, 최대광합성속도도와 순양자수율도 가장 높았다. 수확시기에 따른 단삼뿌리의 생육 및 수량은 큰 차이가 없었으나 salvianolic acid B, cryptotanshinone, tanshinone I, tanshinone IIA의 함량은 수확시기가 늦을수록 유의하게 증가하였으며 salvianolic acid B 함량이 가장 많았으며 수확시기별로는 11월 상순에 비해 이듬해 3월 중순 이후에 수확시료에서 약25.5배 증가하였다. Cryprotanshinone, tanshinone I, tanshinone IIA 함량 또한 2015년 3월 20일 수확한 시료에서 가장 높은 함량을 나타내었다. 따라서 단삼재배에 적합한 온도는 $20^{\circ}C$전후가 적절한 것으로 사료되며 상대적으로 고온조건인 $30^{\circ}C$에서 광합성율, 증산율, 엽록소 형광반응이 크게 저하되므로 서늘한 기후조건인 준고랭지 이상의 지역에서 단삼을 재배하는 것이 유리할 것으로 판단된다. 또한 고품질 단삼 유통을 위한 적정 수확시기는 단삼을 파종한 다음 해 3월 중순 이후에 수확을 하는 것이 합리적인 것으로 사료된다.

• Progress in Superconductivity
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• 제12권2호
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• pp.82-87
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• 2011

We studied the trapped field properties of bulk Y-Ba-Cu-O superconductors by applying 3 T of the permanent or $Nb_3Ti$ superconducting magnet. The 28 mm circular type of YBCO bulk superconductor was prepared and then hole at the center of bulk, parallel to the c-axis, was mechanically drilled. Typical size of hole in YBCO bulk was 10 mm in diameter. In order to examine the trapped field variation in terms of different impregnated materials, a hole in YBCO bulk was filled with resin and indium respectively. The trapped field decay due to flux flow was determined in terms of time. Our preliminary result indicates the trapped field value measured on the YBCO without hole after 30 minute by applying 3 T, was 6,500 G, which is much higher than that, 4,500 G, measured on YBCO with hole. Also, we confirmed that the tendency of a trapped field decrement with time was almost the same regardless of the impregnated materials in YBCO.

• 천문학회지
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• 제41권5호
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• pp.121-137
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• 2008

We present optical and near-infrared imaging and long-slit spectroscopy for the blue compact dwarf galaxy (BCD) Mrk 49 in the Virgo Cluster. The surface brightness distribution analysis shows that Mrk 49 consists of an off-centered blue bright compact core of r = 10" and a red faint outer exponential envelope. The $H_{\alpha}$ image and color difference suggest that these two components have different stellar populations: a high surface brightness population of massive young stars and an underlying low surface brightness population of older stars. The redder near-infrared colors of the inner most region suggest that the near-infrared flux of Mrk 49 originates from evolved massive stars associated with the current star-forming activity. The total apparent magnitude is $B_T\;=\;14.32$ mag and the mean effective surface brightness is ${\mu}_{eff}(B)\;=\;21.56$ mag $arcsec^{-2}$. Long-slit spectroscopy shows that Mrk 49 rotates apparently as a solid body within r = 10" in a plane at position angle 55 degrees with an amplitude of about $20\;km\;sec^{-1}$. The measured radial velocity of Mrk 49 was derived as $1,535\;km\;sec^{-1}$; and the total mass of stars and gases is in the range of 3 to $6\;{\times}\;10^9\;M_{\odot}$. The mass-to-light ratios for the central region of Mrk 49 in I and B band are estimated 1.0 and 0.5, respectively. The upper limit of the dark matter to visible matter ratio seems to be < 5. The oxygen abundance is $12\;+\;\log(O/H)\;=\;8.21\;{\pm}\; 0.1$ which is about one quarter of the solar value while the relative helium abundance appears to be similar to that of the sun.