• 제목/요약/키워드: Component of medium

검색결과 489건 처리시간 0.032초

웹 접근성 강화를 위한 유저 인터페이스 감리 프레임워크 설계 (A Design on the Audit Framework of the User Interface for the Web Accessibility)

  • 김희완;강소영;강재화;김동수
    • 한국컴퓨터정보학회논문지
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    • 제15권4호
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    • pp.107-118
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    • 2010
  • 웹 기반 정보시스템에서의 유저 인터페이스는 사용자가 시스템에 접할 수 있는 매개체이다. 유저 인터페이스는 정보시스템의 접근성과 사용성을 높이는 수단이며, 웹 기반 정보시스템에서의 중요한 핵심 구성요소이다. 이에 본 논문은 웹 기반 정보시스템에서 사용성과 접근성을 강화하는 유저 인터페이스 감리 프레임워크를 기존 정보시스템 감리점검 프레임워크의 3대 축을 준용하여 개발하였다. 먼저 감리시점으로는 국내 주요 웹 개발방법론의 단계 비교 분석을 통해 도출된 분석, UI설계, UI제작, 테스트의 UI중심 프로세스를 정의하였다. 감리영역은 유저 인터페이스를 구성하는 요소의 분석을 통하여 정보, 디자인, 기술로 정의하였고, 감리관점 점검기준은 사용성, 접근성, 호환성으로 정의하였다. 본 논문에서 제안한 프레임워크를 통해 도출된 점검항목을 실제감리가 수행된 사례에 적용해 봄으로써 제안된 프레임워크를 검증하였다.

바이오에탄올 생산을 위한 폐MDF의 전처리 및 효소 당화 (Pretreatment and Enzymatic Saccharification of Wasted MDF for Bioethanol Production)

  • 강양래;황진식;배기한;조훈호;이은정;조영손;남기두
    • KSBB Journal
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    • 제30권6호
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    • pp.332-338
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    • 2015
  • The objective of this study was designed to determine the possibility of bioethanol production from wasted medium density fiberboard (wMDF). We were investigated the enzymatic saccharification characteristics using the enzyme (Cellic CTec3) after pretreatment with sodium chlorite. According to the component analysis results, the lignin contents before and after the pretreatment of wMDF (milling using sieve size of $1,000{\mu}m$) was significantly reduced from 31.13% to 4.11%. Therefore, delignification ratio of pretreated wMDF was found to be up to about 87-89% depending on the sieve size. And we were tested to compare the saccharification ratio according to the sieve size of wMDF ($1,000{\mu}m$, $200{\mu}m$), but it was no significance depending on the sieve size. When enzyme dosage was 5% based on the substrate concentration, enzymatic saccharification ratio was obtained up to 70% by maintaining at $50^{\circ}C$ for 72 hours. We could made the substrate concentration of pretreated wMDF ($1,000{\mu}m$) up to 12% and then enzymatic saccharification ratio was 76.8%, also contents of glucose and xylose were analyzed to 77,750 and 14,637 mg/L, respectively.

PCB의 이온-마이그레이션에 영향을 미치는 주요요인 (Main Factors that Effect on the Ion-Migration of PCB)

  • 장인혁;김정호;오길구;이영주;임홍우;최연옥
    • 한국신뢰성학회지:신뢰성응용연구
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    • 제16권3호
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    • pp.202-207
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    • 2016
  • Purpose: The purpose of this study is main factors (environmental conditions, pattern spacing, pattern material) that effect the ion-migration of PCB. Methods: Recently, the electronic components are becoming more high density of electronic device, so that electronic circuits have smaller pitches between the patten and more vulnerable to insulation failure. so the reliability of electric insulation of device has become an ever important issue as device contact pitches of pattern. Usually, ion-migration occurs in high temperature and high humidity environment as voltage is applied to the circuit. Under high temperature and high humidity, voltage applied electronic components respond to applied voltages by metals's electrochemical ionization and a conducting filament forms between the anode and cathode across a nonmetallic medium. This leads to short-circuit failure of the electronic component. Results: we studied ion-migration that occurs in accordance with the main factors (environmental conditions, pitches, pattern material). The PCB pattern material was made by two different types of material (free solder, OSP) for this research and pitches of pattern is 0.15mm, 0.3mm, 0.5mm. PCB was experimented in the environmental conditions (high temperature $120^{\circ}C$, high temperature and high humidity $85^{\circ}C$, 85%RH) and was analyzed for ion-migration through the experiment results. Conclusion: We confirmed that environmental condition, pitches of pattern, pattern material had effect on ion-migration of PCB.

A new steel panel zone model including axial force for thin to thick column flanges

  • Mansouri, Iman;Saffari, Hamed
    • Steel and Composite Structures
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    • 제16권4호
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    • pp.417-436
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    • 2014
  • During an earthquake, steel frame columns can be subjected to high axial forces combined with inelastic rotation demand resulting from story drift. Generally, the whole beam or component can be represented with one element. In elasto-plastic analysis, subdivision is necessary if the plastic deformation occurs within two ends of beams. If effects of the joint panel are necessarily considered in the analysis, the joint panel should be represented with an independent element. It is a special element to represent the shear deformation of the joint panel in the beam-column connection zone. Several analytical models for panel zone (PZ) behavior exist, in terms of shear force-shear distortion relationships. Among these models, the Krawinkler PZ model is the most popular one which is used in the AISC code. Some studies have pointed out that Krawinkler's model gives good results for the range of thin to medium column flanges thickness. This paper, introduces a new model to estimate the response of shear force-shear distortion for the PZ including column axial force. The model is applicable to both thin and thick column flange. To achieve an appropriate PZ mathematical model first, the effects of PZ strength and stiffness on connection response are parametrically studied using finite element models. More than one thousand and four-hundred beam-column connections are included in the parametric study, with varied parameters; then based on analytical results a simple mathematical model is presented. A comparison between the results of proposed method herein with FE analyses shows the average error especially in thick column flange is significantly reduced which demonstrates the accuracy, efficiency, and simplicity of the proposed model.

한해성 품종 종묘생산을 위한 로티퍼의 적정 영양강화 수온 및 미세조류 선택 (Optimal Enrichment Temperature for Rotifer and Microalgae Selection for Cold-Water Species Culture)

  • 박진철;이배익;박흠기;권오남
    • 한국수산과학회지
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    • 제43권6호
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    • pp.654-658
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    • 2010
  • The purpose of this study is to establish methods for enhancing the survival and growth of cold-water fish and crustacean larvae based on the nutritional components of zoo and phyto live foods. Rotifers, Brachionus rotundiformis, were cultured with a supplement of freshwater condensed Chlorella vulgaris at $28^{\circ}C$ and enriched with Algamac $2000^{(R)}$ at 16, 20 and $26^{\circ}C$, respectively. Isochrysis galbana, Chaetoceros calcitrans and Chlorella ellipsoidea were centrifuged for component analysis after being cultured for approximately one week with conway medium at $20^{\circ}C$. The crude protein and lipid contents of the rotifers were 58.4% and 10.9%, respectively, before enrichment. After enrichment at each temperature, total protein and essential amino acid contents were increased by reducing the enrichment temperature. However, unsaturated fatty acids and multiple fatty acid index (UI) showed their highest values at $20^{\circ}C$. Mono-unsaturated fatty acid content was highest (72.6%) at $16^{\circ}C$. The total protein contents of C. calcitrans and C. ellipsoidea were higher, 33.0% and 35.2%, respectively, than that of I. galbana, 27.8%. Methionin, leusine and histidine, essential amino acids of C. ellipsoidea, had considerably higher values, 50.2, 287.2 and 68.1 mg/g dry matter, respectively, compared to other microalgae. Total lipids, UI, DHA and n-3 PUFA of I. galbana had higher values, 23.6, 272.0, 12.9% and 45.2%, respectively, than other microalgae. Therefore, for cold-water fish and crustacean larvae that require high n-3 PUFA and DHA contents, enrichment of rotifers is desirable at $20^{\circ}C$. Fish larvae would also need more I. galbana than other microalgae.

Line Profiles of the Saturn Ring Planetary Nebula

  • 이성재;형식
    • 천문학회보
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    • 제36권2호
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    • pp.115.1-115.1
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    • 2011
  • We analyzed the line profiles of the planetary nebula (PN) NGC 7009 secured with the Keck I HIES and BOES's spectral data. The 5 positions were taken over the nebular image, 4 points on the bright rim plus 1 point at the central position. The covered spectral wavelength range was $3250{\AA}-8725{\AA}$ in these observations. We decomposed the lines of HI, HeI, HeII, CII, NIII, [ClIII], [NII], [OII], [OIII], [SII], [SIII], [ClIII], and [ArIII] using the IRAF and StarLink/Dipso. After correcting the Earth's movement and the PN's radial velocities, -48.6 & -48.9 km/s, respectively, for the Keck & BOES, we produced the line profiles in a velocity scale. The zero velocity at each line profile clearly indicates which part of the components is approaching or receding, giving a general information of the kinematical structure. Almost all of the low-to-medium excitation lines, such as [NII], [SII], [O III], and [ArIII], secured at the central position and four positions along the major & minor axes, showed 3 components, double peak + a wide wing component, suggesting the fast outflow structures are present. The overall geometry is a prolate shell which also has a fainter outer shell in the halo zone, but there appears to be some peculiar sub-structures inside the main shell. The high excitation He I, HeII, NIII lines which might be formed close to the inner boundary of the shell show unusual features, completely different from the other lines. The HeII and these high excitation lines may be indicative of a relative recent fast outflow from the central star and the permitted lines such as NIII might be affected by the innermost structure. We discuss a possible presence of a jet-like fast outflow structure in an out-flow axis different from the main axis of the spheroid shell.

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옥수수 깜부기균에 의한 페닐알라닌의 대사적 분해 (Metabolic Fate of Phenylalanine in the Corn Smut Fungus Ustilago maydis)

  • 현민우;김성환
    • 한국균학회지
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    • 제39권3호
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    • pp.249-253
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    • 2011
  • Ustilago maydis(옥수수깜부기균)에 있어서 동포자 melanin의 구성성분으로 catecol 계 알려진바 이 물질의 전구체인 benzoic acid의 생성 여부와 그 유래 원천을 추적하고자 phenylalanine의 분해 과정을 조사하였다. 방사성 동위원소가 표지된 L-$^{14}C$-phenylalanine 및 $^{14}C$-trans-cinnamic acid를 첨가한 액체배지에서 균체와 배양액을 대상으로 대사산물을 추적 조사한 결과 trans-cinnamic acid, benzoic acid, 4-hydroxybenzoic acid와 hydroxybenzoic acid derivatives 추정되는 물질 등이 검출되었다. 또한 L-$^{14}C$-phenylalanine을 대사하여 매우 천천히 공기 중으로 $^{14}CO_2$를 방출함을 확인하여 phenylalanine을 완전히 분해 할 수 있음을 밝혔다. 결론적으로 본 연구는 옥수수깜부기균이 benzoic acid를 생성하고 그 유래는 phenylalanine의 분해에서 만들어지는 증거를 제시하였다.

참여기체를 가진 무한 원형관 계의 복사 열전달 증진 (Augmentation of Radiative Heat Transfer in an Infinite Cylindrical Pipe Enclosing a Participating Gas)

  • 변기홍
    • 대한기계학회논문집
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    • 제16권10호
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    • pp.1955-1962
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    • 1992
  • 본 연구에서는 무한 원형관 안의 복사에 참여하는 참여가스에 면을 도입시키 면, 참여가스로부터 원형관 벽면으로의 복사 열유속(radiatve heat flux)이 증진 또는 감소되는 현상을 연구하는 데 있다. 참여가스는 흡수, 방사 특성이 온도와 파장에 변하지 않는 회체가스(gray gas)이거나, 화석 연료 연소시 연소가스의 성분이며, 복사 에 참여하는, 수증기와 이산화탄소의 혼합물이다. 편의상, 이 가스를 실제가스(real gas)라 부르기로 한다.도입면은 동축 무한 원형관(coaxial Infinite cylinder)이다. 참여가스의 성분, 계의 직경, 동축 무한 원형관 사이의 직경비, 면의 방사율, 면과 가 스의 온도가 열전달 증진에 미치는 영향을 연구하고자 한다.

된장에서 분리한 효모(Pichia farinosa NASS-2)의 돈분 악취감소효과 (Decrease efficiency of Offensive Odor from Pig Excreta by Yeast Strain, Pichia farinosa NASS-2 Isolated from Soy Bean Paste)

  • 유재홍;박인철;김완규
    • 한국균학회지
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    • 제40권4호
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    • pp.254-257
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    • 2012
  • 경기도 지방의 된장 시료로부터 악취감소 효과 미생물 중에서 효모가 분리되었으며 rDNA염기서열분석에 의하여 Pichia farinosa로 동정 되었다. 공시균주 P. farinosa NASS-2로 대량배양조건 확립 및 미생물처리제를 제조하였다. 분리한 효모로 제조한 악취저감효과 처리제의 실내 시험결과 돈분에 미생물제를 처리하고 15일 경과 후 악취가스 감소율을 조사한 결과, 암모니아가스($NH_3$ gas)는 처리 전 19.49 ppm에서 처리 후는 1.38 ppm으로, 황화수소가스($H_2S$ gas)는 처리 전 5.89 ppb에서 처리 후는 0.32 ppb으로 감소하는 효과를 나타내었다. 일반적으로 박테리아가 악취저감효과 미생물로 사용되고 있으나 본 연구에서 사용한 된장에서 분리한 효모 특히 산막효모인 P. farinosa NASS-2의 악취효과(암모니아가스, 황화수소 가스)는 처음 보고이다.

Three-Dimensional Numerical Magnetohydrodynamic Simulations of Magnetic Reconnection in the Interstellar Medium

  • TANUMA SYUNITI;YOKOYAMA TAKAAKI;KUDOH TAKAHIRO;SHIBATA KAZUNARI
    • 천문학회지
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    • 제34권4호
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    • pp.309-311
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    • 2001
  • Strong thermal X-ray emission, called Galactic Ridge X-ray Emission, is observed along the Galactic plane (Koyama et al. 1986). The origin of hot ($\~$7 keV) component of GRXE is not known, while cool ($\~$0.8 keV) one is associated with supernovae (Kaneda et al. 1997, Sugizaki et al. 2001). We propose a possible mechanism to explain the origin; locally strong magnetic fields of $B_{local}\;\~30{\mu}G$ heat interstellar gas to $\~$7 keV via magnetic reconnection (Tanuma et al. 1999). There will be the small-scale (< 10 pc) strong magnetic fields, which can be observed as $(B)_{obs} \;\~3{\mu}G$ by integration of Faraday Rotation Measure, if it is localized by a volume filling factor of f $\~$ 0.1. In order to examine this model, we solved three-dimensional (3D) resistive magnetohydrodynamic (MHD) equations numerically to examine the magnetic reconnect ion triggered by a supernova shock (fig.l). We assume that the magnetic field is Bx = 30tanh(y/20pc) $\mu$G, By = Bz = 0, and the temperature is uniform, at the initial condition. We put a supernova explosion outside the current sheet. The supernova-shock, as a result, triggers the magnetic reconnect ion, and the gas is heatd to > 7 keV. The magnetic reconnect ion heats the interstellar gas to $\~$7 keV in the Galactic plane, if it occurs in the locally strong magnetic fields of $B_{local}\;\~30{\mu}G$. The heated plasma is confined by the magnetic field for $\~10^{5.5} yr$. The required interval of the magnetic reconnect ions (triggered by anything) is $\~$1 - 10 yr. The magnetic reconnect ion will explain the origin of X-rays from the Galactic ridge, furthermore the Galactic halo, and clusters of galaxies.

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