• 한국가구학회지
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• 제12권1호
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• pp.39-45
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• 2001

This study was carried out to evaluate the feasibility of using HDF as surface panels as well as core materials for flush door manufacturing. Several core compositions were developed and applied to manufacture door specimens. Core materials were tested under bending load, door manufacturing process was analysed to find better way of using HDF for door manufacturing, and door specimens were tested under bending, twisting and impact loads. From this study, it was concluded that HDF can be used to manufacture quality flush doors. And it was desirable to use light color HDF as surface panels because dark color HDF caused a problem in manufacturing process by shadow shown through finishing veneer. HDF doors were light, and showed good quality and higher resistance against bending twisting and impact loads.

• 한국문헌정보학회지
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• 제54권4호
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• pp.261-281
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• 2020

다크 아카이브를 통해 다양한 유형의 전자기록물을 장기적으로 보존하는 활동은 그 중요성이 점차 증대하고 있으나, 현재 다크 아카이브에서는 전자기록물 장기보존을 위한 최적화된 정보패키지 구조가 마련되어 있지 않다. 이에 본 연구에서는 다크 아카이브의 핵심적인 프로세스를 중심으로 OAIS 참조모델 정보패키지를 재구성하여 4개의 카테고리를 제안하였다. 각 카테고리의 세부 기술항목은 OAIS 참조모델, ISO 23081, 기록관리 메타데이터 표준, ISAD(G), ISAAR(CPF), ISDF, ISDIAH를 기반으로 총 4개의 상위요소와 27개의 하위요소로 구성하였다. 이는 다크 아카이빙에 최적화된 정보패키지 구성의 기반으로 활용될 수 있으며, 전자기록물의 장기 보존을 보다 효율적으로 지원할 수 있을 것으로 기대된다.

• 천문학회보
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• 제32권1호
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• pp.40.2-40.2
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• 2007

• 천문학회보
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• 제40권2호
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• pp.41.4-42
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• 2015

Outflows and jets from young stellar objects (YSOs) are prominent observational phenomena in star formation process. Indicating currently ongoing star formation and directly tracing mass accretion, they provide clues about the accretion processes and accretion history of YSOs. While outflows of low-mass YSOs are commonly observed and well studied, such studies for high-mass YSOs have been so far rather limited owing to their large distances and high visual extinction. Recently, we have found a number of molecular hydrogen (H2 1-0 S(1) at 2.12 micron) outflows in the long, filamentary infrared dark cloud (IRDC) G53.2 located at 1.7 kpc from UWISH2, the unbiased, narrow-band imaging survey centered at 2.12 micron using WFCAM/UKIRT. In IRDC G53.2 which is an active star-forming region with ~300 YSOs, H2 outflows are ubiquitously distributed around YSOs along dark filaments. In this study, we present the most prominent H2 outflow among them identified in one of the IRDC cores MSXDC G53.11+00.05. The outflow shows a remarkable bipolar morphology and has complex structures with several flows and knots. The outflow size of ~1 pc and H2 luminosity about ~1.2 Lsol as well as spectral energy distributions of the Class I YSOs at the center suggest that the outflow is likely associated with a high-mass YSO. We report the physical properties of H2 outflow and characteristics of central YSOs that show variability between several years using the H2 and [Fe II] images obtained from UWISH2, UWIFE and Subaru/IRCS+AO188 observations. Based on the results, we discuss the possible origin of the outflow and accretion processes in terms of massive star formation occurring in IRDC core.

• 스마트미디어저널
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• 제11권10호
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• pp.46-53
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• 2022

오늘날 4차 산업 혁명과 대규모 R&D 지원으로 인해 국내 기업은 세계 기술력 수준의 산업기술을 보유하기 시작하였으며 중요한 자산으로 변모하였다. 국가는 기업의 중요한 산업기술을 보호하고자 국가핵심기술로 지정하였으며, 특히 원자력, 조선, 반도체와 같은 기술이 유출될 경우 해당 기업뿐만 아니라 국가 차원에서도 심각한 경쟁력 손실로 이어질 수 있다. 매년 내부자 유출, 랜섬웨어 그룹의 해킹공격, 산업스파이에 산업기술 탈취 시도가 증가하고 있으며, 탈취된 산업기술은 다크웹 환경에서의 은밀하게 거래가 이루어진다. 본 논문에서는 다크웹 환경에서 은밀하게 이루어지는 산업기술 유출을 탐지하는 시스템을 제안한다. 제안된 모델은 먼저 OSINT 환경에서 수집한 정보를 이용하여 다크웹 크롤링을 통한 데이터베이스를 구축한다. 이후 KeyBERT 모델을 이용한 산업기술 유출 키워드를 추출한 후 다크웹 환경에서의 산업기술 유출 징후를 정량적 수치로 제안한다. 마지막으로 식별된 다크웹 환경에서의 산업기술 유출 사이트를 기반으로 PageRank 알고리즘 통한 2차 유출 가능성을 탐지한다. 제안된 모델을 통해 27,317개의 중복 없는 다크웹 사이트를 수집하였으며, 100개의 원자력 특허에서 총 15,028개의 원자력 관련 키워드를 추출하였다. 가장 높은 원자력 유출 다크웹 사이트를 기반으로 2차 유출을 탐지한 결과 12개의 다크웹 사이트를 식별하였다.

• Korean Journal of Chemical Engineering
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• 제35권12호
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• pp.2379-2383
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• 2018

We report a facile one-pot aqueous-phase synthesis of PdAu bimetallic nanoparticles with different Pd/Au ratio. The synthesis was conducted by co-reduction of Pd and Au precursor using ascorbic acid as a reducing agent and in the presence of polyallylamine hydrochloride (PAH). By high-angle annular dark field scanning transmission electron microscopy (HAADF-STEM) and energy-dispersive X-ray spectrometry (EDS) analyses, we found that the synthesized nanoparticles had an onion-like core/shell/shell/shell structure with Au-rich core, Pd-rich shell, Au-rich shell, and Pd shell, respectively. We also investigated the catalytic performance of the synthesized PdAu nanoparticles toward hydrogen peroxide generation reaction.

• 천문학회지
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• 제33권1호
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• pp.37-45
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• 2000

We have investigated the properties of the high-latitude cloud MBM 7 using the 3 mm transitions of CO, CS, HCN, $HCO^+,\;C_3H_2,\;N_2H^+$, and SiO. The molecular component of MBM 7 shows a very clumpy structure with a size of $\le$0.5 pc, elongated along the northwest-southeast direction, perpendicularly to an extended HI component, which could be resulted from shock formation. We have derived physical properties for two molecular cores in the central region. Their sizes are 0.1-0.3 pc and masses 1-2 M$\bigodot$ having an average volume density $\~2{\times}10^3 cm^{-3}$ at the peak of molecular emission. We have tested the stability of the cores using the full version of the virial theorem and found that the cores are stabilized with ambient medium, and they are expected not to be dissipated easily without external perturbations. Therefore MBM 7 does not seem to be a site for new star formation. The molecular abundances in the densest core appear to be much less (by about one order of magnitude) than the 'general' dark cloud values. If the depletions of heavy elements are not significant in the HLCs compared with those in typical dark clouds, our results may suggest different chemical evolutionary stages or different chemical environments of the HLCs compared with dense dark clouds in the Galactic plane.

• Environmental Sciences Bulletin of The Korean Environmental Sciences Society
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• 제1권2호
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• pp.69-80
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• 1997

Effects of light on leaf senescence of Phaseolus vulgaris were investigated by measuring the disassembly of chlorophyll-protein complexes in detached leaves which had been kept in the dark or under light. The loss of chlorophyll accompanied by degradation of chlorophyll-protein complexes. PSI (photosystem I) complex containing LHCI (light harvesting complex of PSI) apoproteins was rapidly decreased after the early stage of dark-induced senescence. RC(reaction center)-Core3 was slightly increased until 4 d and slowly decreased thereafter. As disassembly of LHCII trimer progressed after the late stage of senescence, there was a steady increase in the relative amount of SC(small complex)-2 containing LHCII monomer. On the other hand, white and red light adaptation caused the structural stability of chlorophyll-protein complexes during dark-induced senescence. Particularly, red light was more effective in the retardation of LHCII breakdown than white light, whereas white light was slightly effect in protecting the disassembly of PSI complex compared to red light. These results suggest, therefore, that light may be a regulatory factor for stability of chlorophyll-protein complexes in the senescent leaves.

• 천문학회지
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• 제25권1호
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• pp.1-9
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• 1992

We present new approach to analysis of velocity data of globular clusters. Maximum likelihood method is applied to get model parameters such as central potential, anisotropy radius, and total mass fractions in each mass class. This method can avoid problems in conventional binning method of chi-square. We utilize three velocity components, one from line of sight radial velocity and two from proper motion data. In our simplified scheme we adopt 3 mass-component model with unseen high mass stars, intermediate visible stars, and low mass dark remnants. Likelihood values are obtained for 124 stars in M13 for various model parameters. Our preferred model shows central potential of $W_o=7$ and anisotropy radius with 7 core radius. And it suggests non-negligible amount of unseen high mass stars and considerable amount of dark remnants in M13.

• 천문학회보
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• 제41권2호
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• pp.60.1-60.1
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• 2016

To obtain a reliable estimate of the cold dark matter (CDM) substructure mass function in a dense cluster environment, one needs to understand how long a merged halo can survive within the host halo. Measuring disruption time scale of merged halos in a dense cluster environment, we attempt to construct the realistic CDM mass function that can be compared with stellar mass functions to get a stellar-to-halo mass ratio. For this, we performed a set of high-resolution simulations of cold dark matter halos with properties similar to the Virgo cluster. Field halos outside the main halo are detected using a Friend-of-Friend algorithm with a linking length of 0.02. To trace the sub-halo structures even after the merging with the main halo, we use their core structures that are defined to be the most 10% bound particles.