• 한국광물학회지
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• 제13권3호
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• pp.147-163
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• 2000

The mineralogy and chemical composition of reddish to brownish yellow residual soils, so called "Hwangto" have been examined according to representative host rocks. The result of the study indicates that Hwangto consists of 40-80% clay minerals and various minerals such as quartz, feldspar, hornblende, goethite, and gibbsite. Clay minerals include kaolinite, halloysite, illite, hydroxy interlayered vermiculite (HIV), mica/vermiculite interstratifield mineral and chlorite. The mineralogical constituents and contents of Hwangto were different depending on the types of host rocks. Moreover, the Jurassic granitic rocks contain relatively more kaolin minerals, whereas the Cretaceous granitic rocks contain more HIV and illite. In addition, reddish Hwangto contains relatively more kaolinite and HIV, and yellowish Hwangto contains more illite and halloysite. It is suggested that feldspars and micas of host rocks were chemically weathered into illite, halloysite, illite/vermiculite interstratified minerals, and HIV, and finally into kaolinite. Compared with their host rocks, the major chemical compositions of Hwangto tend to contain more $Al_2O_3,\;Fe_2O_3,\;H_2O$ in amount and less Ca, Mg, and Na. Hwangto contains relatively high amount of trace elements, P, S, Zr, Sr, Ba, Rb, and Ce including considerable amount of Li, V, Cr, Zn, Co, Ni, Cu, Y, Nb, La, Nd, Pb, Th in excess of 10 ppm. Relatively high amount of most trace elements were detected in the Hwangto. The major and minor chemical compositions of the Hwangto were different depending on the types of host rocks. However, their difference was in the similar range compared with the compositions of host rocks.

• 한국농촌건축학회논문집
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• 제25권4호
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• pp.9-16
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• 2023

In this study, the status and characteristics of fine dust and its impact on neighboring areas were investigated to proactively respond to the government's environmental regulations expected in the future and to minimize the damage by the fine dust generated at construction waste intermediate treatment plants. In addition, since there are no such plants that can affect the surroundings with no houses or other waste treatment sites nearby, an independently located construction waste intermediate treatment plant was selected to compare the characteristics of fine dust with that from the construction waste intermediate treatment sites located in the downtown area. The conclusions of the study are as follows. (1) The measurement results of PM10 at 4 points in the plant showed that the location where the crushing facility was operating had an elevated level of fine dust at 80㎍/m³ on average and a maximum of 124㎍/m³, and the level rose to 110㎍/m³ at points where vehicles frequent. (2) The PM2.5 measurement results inside the plant showed that the average concentration of the reference point was 16㎍/m³ and the maximum value was 20㎍/m³, which was distributed within the management standard. (3) It was found that the average concentration of PM10 in the nearby area ranged from 28 to 38㎍/m³, which was similar to or lower than 36㎍/m³ of the reference point. Therefore, the concentration of the fine dust generated in the plant had a negligible effect on the increase in concentration of fine dust in nearby areas. (4) The heavy metal contents were measured from the filter paper collected from the plant. The PM10 was found to be about 14 to 26ng/m³, and PM 2.5 was 25 to 28ng/m³, which was the average of domestic atmospheric concentrations. (5) The SEM-EDX analysis results showed that the PM10 contained Si and O around 40% similarly for both. The SiO2, a component of silica occupied the most and C was present as CaCO3, which was assumed to be a limestone component. The remaining components included NaO, Al2O3, and CaO as trace oxides. (6) The SEM-EDX analysis results showed that the PM 2.5 contained 5 to 7% of Cl, which is a chlorine ion, and a small amount of K was detected at 2.51% in the sample from the shutdown plant.

• 한국태양에너지학회:학술대회논문집
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• 한국태양에너지학회 2012년도 춘계학술발표대회 논문집
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• pp.267-273
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• 2012

Solar reforming of methane with CO2 was successfully tested with a direct irradiated absorber on a parabolic dish capable of 5kWth solar power. And the new type of double-layer absorber-the front layer, porous metal foam which absorbs the radiation and transfers the heat from material to gas, and the back layer, catalytically-activated metal foam-was prepared, and its activity was tested by using electric furnace. Ni was applied as the active metal on the gamma-Al2O3 coated Ni metal foam for the preparation of the catalytically-activated metal foam layer. Compared to conventional direct irradiation of the catalytically activated metal foam absorber, this new type of double layer absorber is found to exhibit a superior reaction and thermal storage performance at the fluctuating incident solar radiation. In addition, unlike direct irradiation of the foam absorber, double layer absorber has better thermal resistance, which prevents the emergence of cracks caused by mechanical or thermal shock. The total solar power absorbed reached up to 3.25kW and the maximum CH4 conversion was almost 59%.

• 한국태양에너지학회:학술대회논문집
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• 한국태양에너지학회 2011년도 추계학술발표대회 논문집
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• pp.80-86
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• 2011

Solar reforming of methane with CO2 was successfully tested with a direct irradiated absorber on a parabolic dish capable of 5kWth solar power. And the new type of double-layer absorber - the front layer, porous metal foam which absorbs the radiation and transfers the heat from material to gas, and the back layer, catalytically-activated metal foam - was prepared, and its activity was tested by using electric furnace. Ni was applied as the active metal on the gamma-Al2O3 coated Ni metal foam for the preparation of the catalytically-activated metal foam layer. Compared to conventional direct irradiation of the catalytically activated metal foam absorber, this new type of double layer absorber is found to exhibit a superior reaction and thermal storage performance at the fluctuating incident solar radiation. In addition, unlike direct irradiation of the foam absorber, double layer absorber has better thermal resistance, which prevents the emergence of cracks caused by mechanical or thermal shock. The total solar power absorbed reached up to 3.25kW and the maximum CH4 conversion was almost 59%.

• 청정기술
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• 제28권3호
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• pp.218-226
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• 2022

최근 선진국들은 수소경제 및 탄소중립 사회로의 전환을 위해 수소에너지의 수요가 급격히 증가하고 있으며, 이산화탄소(CO₂)를 배출이 없는 친환경적인 수소(H₂) 생산 기술에 대한 관심이 높아지고 있다. 본 연구에서는 암모니아(NH₃) 분해 수소 제조를 위해 루테늄 알루미나(Ru/Al₂O₃) 분말 촉매와 함께 알루미나 졸(alumina sol)의 무기바인더(inorganic binder)와 메틸 셀룰로오스(methyl cellulose)의 유기바인더(organic binder)를 사용하여 딥 코팅(dip coating) 방법으로 루테늄 알루미나 메탈 모노리스 코팅 촉매를 제조하였다. 딥 코팅을 위한 촉매 슬러리의 최적 비율로 촉매와 무기바인더의 중량 비율을 1:1로 고정하여 유기바인더 0.1일 때 1회 딥 코팅 시 촉매 코팅양은 61.6 g L^-1이다. 이때 메탈모노리스 표면에 코팅된 촉매 층의 균일한 두께 (약 42 ㎛)와 결정상을 주사전자현미경(Scanning Electron Microscope, SEM)과 X-ray 회절분석(X ray diffraction, XRD)을 통해 확인하였다. 또한, 암모니아 분해 수소 제조의 최적 공정조건을 찾고자 반응표면분석법(Response Surface Method, RSM)을 이용하여 반응온도와 공간속도의 독립변수에 따른 암모니아 전환율에 대한 수치 최적화 회귀식 모델을 계산하였다. 이러한 결과로부터 암모니아 분해 수소생산을 위한 상업적 규모의 공정운전 기본설계 자료로 활용이 가능하다.

• 한국자기학회:학술대회 개요집
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• 한국자기학회 2002년도 동계연구발표회 논문개요집
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• pp.158-159
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• 2002

스핀 밸브에서는 NiFe, CoFe, Cu등 주요 금속들이 면심입방체(111)로 배향이 용이하지만, 자기 터널 접합 소자에서는 $Al_2$O$_3$ 장벽층이 비정질로서 상부 강자성 전극이 충분히 (111) 배향을 할 수 없기 때문에 top bias 방식의 사용이 거의 불가능하며, bottom bias의 경우에도 교환 바이어스의 크기는 상대적으로 작다[1]. 이를 극복하기 위해 인공 초격자를 이용한 인공 반강자성층(synthetic antiferromagnet - SAF)을 이용하여 높은 교환 바이어스 효과를 구현하고자 하였다. (중략)

• 한국전기전자재료학회논문지
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• 제16권2호
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• pp.102-107
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• 2003

This study puts focus on the optimization of growth temperature of CIGS absorber layer which affects severely the performance of solar cells. The CIGS absorber layers were prepared by three-stage co-evaporation of metal elements in the order of In-Ga-Se. The effect of the growth temperature of 1st stage was found not to be so important, and 350$^{\circ}C$ to be the lowest optimum temperature. In the case of growth temperature at 2nd/3rd stage, the optimum temperature was revealed to be 550$^{\circ}C$. The XRD results of CIGS films showed a strong (112) preferred orientation and the Raman spectra of CIGS films showed only the Al mode peak at 173cm$\^$-1/. Scanning electron microscopy results revealed very small grains at 2nd/3rd stage growth temperature of 480$^{\circ}C$. At higher temperatures, the grain size increased together with a reduction in the number of the voids. The optimization of experimental parameters above mentioned, through the repeated fabrication and characterization of unit layers and devices, led to the highest conversion efficiency of 15.4% from CIGS-based thin film solar cell with a structure of Al/ZnO/CdS/CIGS/Mo/glass.

• 암석학회지
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• 제12권4호
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• pp.170-183
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• 2003

북동 발틱 순상지의 데본기 콜라 알칼리 암석구의 일부에 해당하는 속리복합체는 암맥상으로 산출되는 다양한 규모의 초염기성 림프로파이어를 동반한다. 속리 초염기성 럼프로파이어(lamprophyre)는 암석학적 그리고 지구화학적 특성에 의해 아이리카이트(aillikite)로 분류된다. 속리 아아리카이트가 갖는 높은 Cr과 Ni 함량 그리고 낮은 $Al_2$O$_3$ 함량은 이 암석이 결핍된 맨틀의 하쯔버자이트(harzburgite)로부터 유래되었음을 지시한다. 그러나 킴벌라이트(kimberlite)와 비교하면 Cr, Ni의 한량과 mg-number가 낮고 중희토류원소의 결핍정도가 약한 특징을 보이는데, 이는 기원맨틀의 석류석 함량이 적었고 따라서 용융심도도 킴벌라이트보다 앝았다는 것을 지시한다. 속리 아이리카이트에 함유된 매우 높은 불호정성원소들과 휘발성 성분(주로 $CO_2$)은 근본적으로 결핍된 기원맨틀에 부화된 물질이 첨가되어야 함을 지시한다. 또한 속리 아이리카이트의 특징적으로 높은 K함량으로부터 기원맨틀에 금운모 같은K함량이 높은 광물이 존재하였을 것이라고 추정할 수 있다.

• 한국진공학회:학술대회논문집
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• 한국진공학회 2015년도 제49회 하계 정기학술대회 초록집
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• pp.193.1-193.1
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• 2015

실리콘 (Si) 기판 위에 고품질의 갈륨질화물 (GaN) 박막을 성장시키기 위한 노력이 계속되고 있다. 실리콘 기판은 사파이어 기판 보다 경제적인 측면에서 유리하고, 실리콘 직접화 공정에 GaN 소자를 쉽게 접목 가능하다는 장점이 있다. GaN 박막은 2차원 전자 가스형성을 통한 고속소자, 직접 천이형 밴드갭을 이용한 발광소자 및 고전압 소자로써 활용 가능한 물질이다. 종래에는 Si(100) 및 Si(111) 기판 위에 GaN 박막 성장에 대한 연구가 주로 진행되었다. 하지만 대칭성과 격자 불일치도 등 결정학적 특성을 고려할 때 Si(100) 기판 위에 고품질의 GaN 박막을 성장시키는 것은 쉽지 않다. Si(111) 기판은 실리콘 소자 직접화 공정에 적합하지 못한 단점을 가지고 있다. 반면, 최근 Si(110) 기판 위에서 비등방적 변형 제어를 통한 고품질 GaN 박막 성장이 보고 되어 실리콘 집적 소자와 결합한 고전압 소자 및 고속소자 구현에 관한 연구가 진행되고 있다. 본 연구에서는 투과전자현미경 연구를 바탕으로 Si(110) 기판 위에 성장된 GaN의 미세구조에 관한 연구를 소개한다. 열팽창계수의 차이에 의한 GaN 박막 내 결함 생성을 줄이기 위하여 AlN 완충층이 사용되었다. GaN 박막을 암모니아 ($NH_3$) 유량이 다른 조건에서 성장시킴으로써 GaN 박막 미세구조의 암모니아 유량 의존성에 관한 연구를 진행하였다. GaN 박막에서 투과전자현미경 연구와 X-ray 회절 연구를 통하여 결함 거동 및 결정성을 확인하였다. $NH_3$ 유랑이 증가함에 따라 GaN의 성장 거동이 3차원에서 2차원으로 변화됨을 관찰하였다. 또한, 전위밀도의 증가도 확인되었다. $NH_3$ 유량이 낮은 경우 GaN 전위는 AlN와 GaN 경계에 주로 위치하고 GaN 표면 근처에는 전위밀도가 감소하였으나, $NH_3$ 유량이 높을 경우 GaN 박막 표면까지 전위가 관통됨을 확인하였다.

• 한국재료학회지
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• 제25권8호
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• pp.386-390
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• 2015

Fe-base superalloy powders with $Y_2O_3$ dispersion were prepared by high energy ball milling, followed by spark plasma sintering for consolidation. High-purity elemental powders with different Fe powder sizes of 24 and 50 mm were used for the preparation of $Fe-20Cr-4.5Al-0.5Ti-O.5Y_2O_3$ powder mixtures (wt%). The milling process of the powders was carried out in a horizontal rotary ball mill using a stainless steel vial and balls. The milling times of 1 to 5 h by constant operation (350 rpm, ball-to-powder ratio of 30:1 in weight) or cycle operation (1300 rpm for 4 min and 900 rpm for 1 min, 15:1) were applied. Microstructural observation revealed that the crystalline size of Fe decreased with an increase in milling time by cyclic operation and was about 15 nm after 3 h, forming a FeCr alloy phase. The cyclic operation had an advantage over constant milling in that a smaller-agglomerated structure was obtained. The milled powders were sintered at $1100^{\circ}C$ for 30 min in vacuum. With an increase in milling time, the sintered specimen showed a more homogeneous microstructure. In addition, a homogenous distribution of Y-compound particles in the grain boundary was confirmed by EDX analysis.