강원도 고성군 오봉리에는 6개의 화산체(뒤배재, 오음산, 갈미봉, 249 m 고지, 166 m 고지, 102 m 고지)가 밀집하여 분포하고 있다. 그리고 고성산 화산체와 운봉산 화산체가 단독으로 멀리 떨어져 있다. 오봉리의 249 m 고지 화산체는 이 연구에서 새롭게 발견된 것이며, 오봉리에 분포하는 6개의 화산체들을 오봉리 화산체군이라 명명한다. 이 지역 화산체는 여러 연구자에 따라 화산전, 플러그 돔, 원통형 화산통 등으로 해석된다. 이 연구는 화산체의 형태, 화산분출물의 층서 및 특징을 바탕으로 화산활동 양상과 화산체의 형성과정을 알아보았다. 이 지역의 모든 화산체는 중생대 화강암 위에 현무암류가 분포하고, 기반암에서 상부로 갈수록 산사면의 경사도가 증가하는 돔 형태이다. 특히 3개의 화산체(뒤배재, 166 m 고지, 102 m 고지)에서는 현무암과 기반암 사이에 화성쇄설층이 발견된다. 뒤배재 화산체의 화성쇄설층에서는 기반암 기원으로 추정되는 석영, 장석 및 화강암편과 화산분출물인 스코리아 암편이 분포한다. 그리고 모든 화산체의 현무암내에는 맨틀포획암과 기반암인 화강암류와 하부지각 기원의 반려암류의 포획암을 함유한다. 또한 각진 형태의 감람석, 사장석, 휘석 등의 포획광물이 있다. 이러한 사실은 마그마가 지표로 빠르게 상승하였고, 화산활동이 폭발적이었음을 지시한다. 또한 현무암내의 다량의 포획광물 등은 현무암질 마그마의 점성을 증가시켜 돔형의 화산체를 형성한 것으로 판단된다. 그리고 화산체가 오랜 시간 동안의 삭박작용을 거쳐 원지형이 파괴되면서, 돔의 심부가 기반암 위에 플러그 돔으로 남게 된 것으로 해석된다.

분화용 거베라의 채종 체계를 확립하기 위하여 ‘Ge- 10-47’(S4) 등 2계통에 대하여 1월부터 12월까지 15일 간격으로 자가수분을 실시하였고, ‘Ge-10-47’ 등 5계통 에 대하여 자가 수분, 형매 교배 및 타가수분 등의 교 배 방법에 따른 결실화율 및 결실화 당 종자 수를 조 사하였다. 교배시기별로는 주간 25 ± 3οC/야간 15 ± 3οC 가 유지되는 4-5월과 9-10월은 결실화율은 80% 이상이 고, 결실화 당 종자 수는 20개에서 70개로 다른 시기 보다 월등히 많았으나 겨울(11-2월) 및 여름(6-8월)에는 수정이 거의 안 되거나 낮게 나타났다. 교배 방법에 따 른 결실화율은 자가수분이 58.2%, 형매 교배는 70.8%, 타가수분은 77.5%이었다. 결실화 당 종자수도 자가수분 이 14.1개, 형매 교배가 19.0개, 타가수분은 22.7개를 나타냈다. 형매 교배 및 타가수분의 결실율이 자가수분 보다 높고, 결실화 당 채종립도 많은 경향이었다. 또한 교배 횟수는 2회가 알맞았고, 계통의 세대가 진전될수록 결실화율 및 결실화 당 종자 수는 현저히 적었다.

A general synthetic method to make Fe3O4-δ (activated magnetite) is the reduction of Fe3O4 by H2 atmosphere. However, this process has an explosion risk. Therefore, we studied the process of synthesis of Fe3O4-δ depending on heat-treatment conditions using FeC2O4·2H2O in Ar atmosphere. The thermal decomposition characteristics of FeC2O4·2H2O and the δ-value of Fe3O4-δ were analyzed with TG/DTA in Ar atmosphere. β-FeC2O4·2H2O was synthesized by precipitation method using FeSO4·7H2O and (NH4)2C2O4·H2O. The concentration of the solution was 0.1 M and the equivalent ratio was 1.0. β-FeC2O4·2H2O was decomposed to H2O and FeC2O4 from 150˚C to 200˚C. FeC2O4 was decomposed to CO, CO2, and Fe3O4 from 200˚C to 250˚C. Single phase Fe3O4 was formed by the decomposition of β-FeC2O4·2H2O in Ar atmosphere. However, Fe3C, Fe and Fe4N were formed as minor phases when β-FeC2O4·2H2O was decomposed in N2 atmosphere. Then, Fe3O4 was reduced to Fe3O4-δ by decomposion of CO. The reduction of Fe3O4 to Fe3O4-δ progressed from 320˚C to 400˚C; the reaction was exothermic. The degree of exothermal reaction was varied with heat treatment temperature, heating rate, Ar flow rate, and holding time. The δ-value of Fe3O4-δ was greatly influenced by the heat treatment temperature and the heating rate. However, Ar flow rate and holding time had a minor effect on δ-value.

In semiconductor manufacturing, the circuit integrity of packaged BGA devices is tested by measuring electrical resistance using test sockets. Test sockets have been reported to often fail earlier than the expected life-time due to high contact resistance. This has been attributed to the formation of Sn oxide films on the Au coating layer of the probe pins loaded on the socket. Similar to contact failure, and known as "fretting", this process widely occurs between two conductive surfaces due to the continual rupture and accumulation of oxide films. However, the failure mechanism at the probe pin differs from fretting. In this study, the microstructural processes and formation mechanisms of Sn oxide films developed on the probe pin surface were investigated. Failure analysis was conducted mainly by FIB-FESEM observations, along with EDX, AES, and XRD analyses. Soft and fresh Sn was found to be transferred repeatedly from the solder bump to the Au surface of the probe pins; it was then instantly oxidized to SnO. The SnO2 phase is a more stable natural oxide, but SnO has been proved to grow on Sn thin film at low temperature (< 150˚C). Further oxidation to SnO2 is thought to be limited to 30%. The SnO film grew layer by layer up to 571 nm after testing of 50,500 cycles (1 nm/100 cycle). This resulted in the increase of contact resistance and thus of signal delay between the probe pin and the solder bump.

Understanding infrared (IR) luminosity is fundamental to understanding the cosmic star formation history and AGN evolution, since their most intense stages are often obscured by dust. Japanese infrared satellite, AKARI, provided unique data sets to probe this both at low and high redshifts. The AKARI performed an all sky survey in 6 IR bands (9, 18, 65, 90, 140, and 160μm ) with 3-10 times better sensitivity than IRAS, covering the crucial far-IR wavelengths across the peak of the dust emission. Combined with a better spatial resolution, AKARI can measure the total infrared luminosity ( LTIR) of individual galaxies much more precisely, and thus, the total infrared luminosity density of the local Universe. In the AKARI NEP deep field, we construct restframe 8μm, 12μm , and total infrared (TIR) luminosity functions (LFs) at 0.15 < z < 2.2 using 4,128 infrared sources. A continuous filter coverage in the mid-IR wavelength (2.4, 3.2, 4.1, 7, 9, 11, 15, 18, and 24μm ) by the AKARI satellite allows us to estimate restframe 8μm and 12μm luminosities without using a large extrapolation based on a SED fit, which was the largest uncertainty in previous work. By combining these two results, we reveal dust-hidden cosmic star formation history and AGN evolution from z = 0 to z = 2.2, all probed by the AKARI satellite.

Starting from an infrared selected GALEX-SDSS-2MASS-AKARI sample of local star forming galaxies, we built mock samples from redshift 0 to 2.5 to investigate star formation rate (SFR) calibrations using WISE luminosities. We find W3 and W4 band fluxes can indicate SFRs with small scatters when the rest-frame wavelengths are longer than ∼6μm . When the wavelength becomes shorter, the observed luminosities are more tightly connected to the emission of old stellar populations than dust, therefore lose the reliability to trace the SFR. The current SFR calibrations are consistent with previous studies.

We investigate the role of galaxy environment in the evolution of individual galaxies through the AKARI observations of the merging galaxy cluster A2255. MIR diagnostics using N3-S11 colors are adopted to select star-forming galaxies and galaxies in transition between star-forming galaxies and quiescent galaxies. We do not find particular enhancement of star formation rates as a function of galaxy environment, reflected in cluster-centric distance and local surface density of galaxies. Instead, the locations of intermediate MIR-excess galaxies (-1.2 < N3 - S11 < 0.2) show that star-forming galaxies are transformed into passive galaxies in the substructures of A2255, where the local surface density of galaxies is relatively high.

The aim of this research is to reveal the spatial distribution of the star formation activity of nearby galaxies by comparing CO molecular emission lines with the large area observation in far-infrared (FIR) lines. We report the imaging observations of NGC 253 by FIR forbidden lines via FIS-FTS and CO molecular lines from low to high excitation levels with ASTE, which are good tracers of star forming regions or photo-dissociation regions, especially spiral galaxies, in order to derive the information of the physical conditions of the ambient interstellar radiation fields. The combination of spatially resolved FIR and sub-mm data leads to the star formation efficiency within galaxy. The ratio between the FIR luminosity and molecular gas mass, LFIR/MH2 , is expected to be proportional to the number of stars formed in the galaxy per unit molecular gas mass and time. Moreover the FIR line ux shows current star formation activity directly. Furthermore these can be systematic and statistical data for star formation history and evolution of spiral galaxies.

Nearby spiral galaxies M101 and M81 are considered to have undergone a galaxy-galaxy interaction. M101 has experienced HI gas infall due to the interaction. With AKARI far-infrared (IR) photometric observations, we found regions with enhanced star forming activity, which are spatially close to regions affected by the interaction. In addition, the relation between the star formation rate (SFR) and the gas content for such regions shows a significant difference from typical spiral arm regions. We discuss possible explanations for star formation processes on a kiloparsec scale and the association with interaction-triggered star formation. We also observed the compact group of galaxies Stephan's Quintet (SQ) with the AKARI Far-infrared Surveyor (FIS). The SQ shows diffuse intergalactic medium (IGM) due to multiple collisions between the member galaxies and the IGM. The intruder galaxy NGC 7318b is currently colliding with the IGM and causes a large-scale shock. The 160 micron image clearly shows the structure along the shock ridge as seen in warm molecular hydrogen line emission and X-ray emission. The far-IR emission from the shocked region comes from the luminous [CII] 158 μm line and cold dust (~ 20 K) that coexist with molecular hydrogen gas. Survival of dust grains is indispensable to form molecular hydrogen gas within the collision age (~ 5 Myr). At the stage of the dusty IGM environment, [CII] and H2 lines rather than X-ray emission are powerful cooling channels to release the collision energy.

Following the first Public Release of the AKARI Point Source catalogues, we have worked on the production of a new far-infrared All-Sky Diffuse mapping product. In this paper we report first results from the All Sky diffuse maps that will shortly be released to the community, based on analysis of data from the Far Infrared Surveyor ( 65 μm − 160 μm ) instrument. These data are likely to have a strong impact on studies of extended structures, and the diffuse ISM.

Morphological control on hydroxyapatite crystals has attractive prospects in research to clarify the effects of crystal planes on biological performance. Hydrothermal processing is known as a typical type of processing for fabricating well-grown crystals with unique morphology. The purpose of the present study is to examine the feasibility of well-crystallized crystals with oriented structures through hydrothermal treatment of calcite. A single crystal of calcite was applied to hydrothermal treatment in a phosphate solution at 160˚C. Rod-shaped hydroxyapatite crystals with micrometer-size were formed on the 100 face of calcite after treatment, while nanometer-sized hydroxyapatite crystals were formed on the (111). The hydroxyapatite crystals formed on each plane were not morphologically changed with increasing treatment periods. An oriented structure of rod-shaped hydroxyapatite was constructed after hydrothermal treatment of 100 planes on the calcite single, while such orientation was not observed on the (111) plane after the treatment. The layer of hydroxyapatite formed on the 100 plane was thicker than that of the (111) plane. The 100 plane of calcite shows a higher reactivity than that of the (111) plane, which results in rapid crystal growth of hydroxyapatite. The difference in the morphology of the formed hydroxyapatite was governed by the reactivity of each crystal plane exposed to the surrounding solution.

2009년 9월 전남 신안군 압해도 지역의 백악기층에서 완벽하게 보존된 공룡알둥지 화석이 발견되었다. 이 연구에서는 압해도 백악기층의 퇴적시기와 공룡들의 활동시기를 밝히기 위하여 이 지층과 동시퇴적구조를 보이는 화산암역, 이 지층을 정합으로 덮는 산성응회암 그리고 이들을 관입하는 산성맥암에 대하여 K-Ar 전암연대측정을 수행하였다. 이 지층에서 관찰되는 화산암은 렌즈상의 역암과 역질이암층의 역으로 발견되며 그 직경은 3-20 cm이다. 이 층에 포함된 공룡알 둥지와 동시퇴적 구조를 보이는 6개의 화산암역을 대상으로 K-Ar 전암연대측정을 실시하였으며, 그 값은 후기 백악기의 세노마니안(97.6±1.9 Ma), 코니아시안(87.6±1.7 Ma), 산토니안(84.5±1.7 Ma), 캄파니안(82.5±1.6, 77.3±1.5, 75.7±1.5 Ma)에 해당한다. 이 백악기층을 부정합으로 덮는 산성응회암에 대하여 동일 조건으로 K-Ar 전암연대를 측정하였으며 그 결과는 캄파니안(79.2±1.6, 77.3±1.5Ma)에 속한다. 상기의 모든 암층을 관입하는 산성맥암에 대한 K-Ar 전암 연대측정 결과는 70.9±1.4 Ma로 캄파니안에 속한다. 압해도지역에 분포하는 백악기층의 퇴적시기와 공룡의 활동시기는 77-83 Ma 사이이며 이 결과는 공룡알을 포함하는 보성 선소층(81 Ma)과 공룡, 익룡 및 물갈퀴 새발자국을 포함하는 해남 우항리층의 형성시기에 대한 지질연대(79-81 Ma) 등이 서로 대비될 가능성을 시사한다.

Two types of nanoclusters, termed Cluster (1) and Cluster (2) here, both play an important role in the age-hardening behavior in Al-Mg-Si alloys. Small amounts of additions of Cu and Ag affect the formation of nanoclusters. Two exothermic peaks were clearly detected in differential scanning calorimetry(DSC) curves by means of peak separation by the Gaussian method in the base, Cu-added, Ag-added and Cu-Ag-added Al-Mg-Si alloys. The formation of nanoclusters in the initial stage of natural aging was suppressed in the Ag-added and Cu-Ag-added alloys, while the formation of nanoclusters was enhanced at an aging time longer than 259.2 ks(3 days) of natural aging with the addition Cu and Ag. The formation of nanoclusters while aging at 100˚C was accelerated in the Cu-added, Ag-added and Cu-Ag-added alloys due to the attractive interaction between the Cu and Ag atoms and the Mg atoms. The influence of additions of Cu and Ag on the clustering behavior during low-temperature aging was well characterized based on the interaction energies among solute atoms and on vacancies derived from the first-principle calculation of the full-potential Korrinaga-Kohn-Rostoker(FPKKR)-Green function method. The effects of low Cu and Ag additions on the formation of nanoclusters were also discussed based on the age-hardening phenomena.

Recently, the demand for the miniaturization of printed circuit boards has been increasing, as electronic devices have been sharply downsized. Conventional multi-layered PCBs are limited in terms their use with higher packaging densities. Therefore, a build-up process has been adopted as a new multi-layered PCB manufacturing process. In this process, via-holes are used to connect each conductive layer. After the connection of the interlayers created by electro copper plating, the via-holes are filled with a conductive paste. In this study, a desmear treatment, electroless plating and electroplating were carried out to investigate the optimum processing conditions for Cu via filling on a PCB. The desmear treatment involved swelling, etching, reduction, and an acid dip. A seed layer was formed on the via surface by electroless Cu plating. For Cu via filling, the electroplating of Cu from an acid sulfate bath containing typical additives such as PEG(polyethylene glycol), chloride ions, bis-(3-sodiumsulfopropyl disulfide) (SPS), and Janus Green B(JGB) was carried out. The desmear treatment clearly removes laser drilling residue and improves the surface roughness, which is necessary to ensure good adhesion of the Cu. A homogeneous and thick Cu seed layer was deposited on the samples after the desmear treatment. The 2,2'-Dipyridyl additive significantly improves the seed layer quality. SPS, PEG, and JGB additives are necessary to ensure defect-free bottom-up super filling.

We investigated the pulpal response to direct pulp capping in rat molar teeth using mineral trioxide aggregate (MTA) and calcium hydroxide (CH). A palatal cavity was prepared in rat maxillary molar teeth. Either MTA or CH was placed on the exposed pulp and all cavities were restored with composite. Rats were sacrificed for histological evaluation after 12 hours and at 2, 7, 14 and 21 days. In both the MTA and CH groups, reparative dentin formation was clearly observed on histology after 14 days. The MTA-capped pulps were found to be mostly free from inflammation, and hard tissue of a tubular consistent barrier was observed. In contrast, in CH-capped teeth, excessive formation of re¬parative dentin toward residual pulp was evident. The pulpal cell response beneath the reparative dentin layer was examined by immunofluorescence using antibodies against DSP. After 2 days, a few DSP immunopositive cells, most of which showed a cuboidal shape, appeared beneath the predentin layer. At 7 days, DSP-immunopositive cells with columnar odontoblast-like cells were seen beneath the newly formed hard tissues. At 14 and 21 days, DSP was more abundant in the vicinity of the odontoblastic process along the dentinal tubules than in the mineralized reparative dentin. The CH group showed strong expression patterns in terms of DSP immunoreactivity. Our results thus indicate that MTA may be a more effective pulp capping material as it induces the differentiation of odontoblast-like cells and the formation of reparative dentin without the loss of residual pulp functions.

Poly(ADP-ribosyl)ation is post-translational modification of cellular proteins related to cell survival, cell death, cellular proliferation and epigenetic events. It has recently been shown to be important for pre-implantation development of mouse embryos. However, its function during early embryonic development of pig is not clear. This study investigated the importance of poly(ADP-ribosyl)ation during in vitro development of pig embryos produced by in vitro fertilization(IVF) or parthenogenetic activation (PA). Results showed that, chemical inhibition of PARP by 3-aminobenzamide (3-AB) did not influence the in vitro development of pig embryos up to morula stage (20±3.1 vs. 28.1±1.2%; p>0.05) but significanlty reduced the rate of blastocyst formation (5.2±2.1 vs. 20±3.1%; p<0.05) when compared to non-treated controls. Furthermore, culture of morula stage embryos in the pressence of 3-AB for 24h significantly reduced the rate of blastocyst formation (19.6± 4.6 vs. 41.4±5.3%; p<0.05) and expansion (4.7±3.0 vs. 28.1±6.1; p<0.05). The proportion of large-sized blastocyst (>200 μm) having higher blastocoel volume (15.3×106 μm3) was significantly reduced (p<0.05) in treatment group (32.2±7.8%) compared to non-treated control group (65.7±9.0%). TUNEL assay revealed that poly(ADP-ribosyl)ation-inhibited blastocyst had significantly increased indices of apoptosis than those of non-treated controls (10.88±0.02 vs. 2.71±0.01; p<0.05). These data suggest that Poly(ADP-ribosyl)ation may be important for blastocyst formation in pig embryo.

한자문화권의 한자문화란 한문을 공용문어로 사용하여 영위된 종합적 지식체제 이다. 즉 한문을 지적 수단으로 사용하였던 사람들의 生活知, 學問知, 普遍知, 構想知등이 모여 이루어진 知識地形圖이다. 한자문화의 ‘知的傳統’은 가치의 역사적 축적이다. 특히 한국의 지적전통은 한 국의 지반에서 현실적으로 갖는 의미라고 할 수 있다. 한자기록으로 이루어진 지 적전통은 다양하게 전개되어 왔으며, 그것을 교육하고 학습하는 분야가 한문과목 이다. 우리의 한문문화를 동아시아 한문문화 속에서 비교하여 그 同異와 變化, 나아 가 普遍化를 분석할 때 우리만의 특성을 찾아낼 수 있다. 본고는 한자문화 중 전 통교육과 관련된 지식형성에 관해서 살펴보았다. 이 때 지식형성에 어떤 교재가 어떤 교육방법으로 사용되었는가를 밝히는 일은 매우 중요하다. 이에 ‘전통’ 한문 교육에서 그 지식의 분류와 지식의 실천내용을 고찰하여 지식형성의 틀을 찾아내고자 하였다. 전통적 몽학 한문교재는 天地人분류체계를 기반으로 지식을 형성하고 있다. 우선 자연에 대한 개괄적 이해를 토대로 하고, 그 위에 이상적 인간의 모습으로서 사회의 질서체제와 예교를 제시하였다. 이러한 분류체계는 고대사회의 식자교재 인 『급취장』을 비롯하여, 가장 널리 사용된『천자문』등의 중국교재는 물론이고, 조선시대의 『유합』이나『訓蒙字會』에서도 찾아볼 수 있다. 이런 분류체계 안에 서 초학자들은 識字와 함께 자연스럽게 전통적 세계관과 인간관에 접하고 수용할 수 있었다. 한편 교화용 교재는 자연에 관한 이해에 앞서 인간에 대한 이해를 다양하게 제 시하고 있다. 중국 宋代에 만들어진 『소학』,『삼자경』의 분류체계가 율곡의 『성학집요』나『격몽요결』등의 계몽서에 수용되어 계승되었다. 이러한 교화용 교재의 분류체계는 학습자로 하여금 심신의 수양과 독서를 통한 자기계발의 학습방법과 사회 속에서의 처신을 체득하게 한다. 이러한 전통적 몽학교재에 보이는 분류체계를 현대 한문교육 교재에 활용하게 되면, 교육과정에서 요구하는 전통의 이해와 계승의 한 방법이 될 것으로 기대한다.

중국어는 중국인의 정신세계의 고향이자 인류의 공동 재산이며, 한자의 전파는 세계 문명에 대한 일종의 책임이다. 한자의 출현은 선인들의 세계에 대한 인식을 부호화하여 표현한 형식이며, 이로 인해 한자의 제자원리는 선인들의 인식론의 지 배를 받으면서 형성된 제자 근거에 기초하고 있다. 때문에 교사의 입장에서 볼 때 한자 교육은 한자의 제자 원리에 근거하여 선인들의 의식을 습득하면서, 최종적으 로 학생들로 하여금 직접 선인들의 인식 방법의 결과를 따르면서 창조된 한자의 구성 원리를 습득하게 하는 것이다. 최근의 이루어지고 있는 한자교육을 보면 한 자의 제자 원리를 학생들 스스로 자각하여 학습하게 하기 보다는 교육 방법에 있 어 기계적이어서 그 효과가 극대화되지 못하고 있어 “한자학습의 어려움”만을 느 끼게 하고 있다. 본문은 중국 대륙에서 시행되고 있는 한자교육의 실상에서 출발 하여 비효율적인 한자교육이 나타나는 현상과 그 원인을 분석하여, 한자교육 중 한자의 제자원리를 존중해야 함을 말하고 있다. 본문은 중국철학, 정치 제도, 경제 조건 등 여러 방면에서 한자의 제자 원리에 나타나고 있는 의식이 한자 교육에 어떤 영향을 미칠 수 있는지 나름의 견해를 밝힘으로써, 전 세계의 한자 교육에 대한 새로운 인식의 틀을 제공함으로써, 흥미와 효과적인 한자교육의 방법을 제시 하고자 한다.