• Title/Summary/Keyword: Ultra Violet

검색결과 408건 처리시간 0.028초

Varification of Phase Defect Correctability of Nano-structured Multilayer for EUV Reflection

  • Lee, Seung-Yoon;Kim, Tae-Geun;Jinho Ahn
    • 한국진공학회지
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    • 제12권S1호
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    • pp.40-45
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    • 2003
  • Ru interfacial layer was inserted into Mo-on-Si interface to enhance the extreme ultra-violet (EUV) reflective multilayer properties. The stacking status and optical properties are analyzed using cross-sectional transmission electron microscope (TEM), and reflectometer. About 1.5% of maximum reflectivity can be acquired as predicted in optical simulation, which is thought to be originated from the diffusion inhibition property. Phase defect correctability of the multilayer can be enhanced by the insertion of Ru barrier layer.

Analysis of the North Galactic Pole region with FIMS

  • 최연주;민경욱;선광일
    • 천문학회보
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    • 제35권1호
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    • pp.71.2-71.2
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    • 2010
  • Cooling hot gas sets a floor on the ionization level for diffuse gas in the ISM in general and the galactic halo. Many high galactic latitude sight lines, cooling hot gas is the dominant source of the ionization. Such sites are prime regions for the formation of both C IV and Si IV ions at a temperature of T~105K. To study of the ISM that have the 104.5~6K ionization state by ionization or photoionization by the collision, searching for the radiation energy that is emitted at far ultra violet range is required. In this paper, we report the analysis of NGP( North Galactic Pole, $l:270^{\circ},b:90^{\circ},rad:40^{\circ}$) region by fuv($1350{\sim}1750{\AA}$) data that are surveyed with FIMS. After making the FIMS FUV image of the NGP region, we divided up into 50 small regions for that and got the spectrum emission lines from each one.

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Analysis of the North Galactic Pole region with FIMS

  • 최연주;민경욱;선광일
    • 천문학회보
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    • 제35권2호
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    • pp.70.2-70.2
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    • 2010
  • Cooling hot gas sets a floor on the ionization level for diffuse gas in the ISM in general and the galactic halo. Many high galactic latitude sight lines, cooling hot gas is the dominant source of the ionization. Such sites are prime regions for the formation of both C IV and Si IV ions at a temperature of T~105K. To study of the ISM that have the 104.5~6K ionization state by ionization or photoionization by the collision, searching for the radiation energy that is emitted at far ultra violet range is required. In this paper, we report the analysis of NGP(North Galactic Pole, $l:0^{\circ},b:90^{\circ}$,rad: $40^{\circ}$) region by fuv($1350\sim1750\AA$) data that are surveyed with FIMS. After making the FIMS FUV image of the NGP region, we divided up into some small regions for that and got the spectrum emission lines from each one.

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UV/TiO2에 의한 수용성 염료의 분해에 관한 연구 (A Study on the Decomposition of Water Soluble Dyes by UV/TiO2)

  • 정갑섭
    • 한국환경과학회지
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    • 제12권3호
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    • pp.319-324
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    • 2003
  • The characteristics of photocatalytic decomposition of dye waste water by titanium dioxide was studied in a batch reactor under constant strength of ultra-violet ray. The decomposition rate of methyl orange by TiO$_2$ was pseudo-first order, anatase type TiO$_2$ was more effective than rutile type below the dosage of 5g. The decomposition rate was increased with decreasing initial pH, increasing reaction temperature and oxidant concentration. The decomposition rate of water soluble dyes was decreased in order of rhodamine B>eosin Y>methyl orange.

건축물 외부 중공벽의 시공방안에 관한 연구 - 외부 점토벽돌의 사용을 중심으로 - (A study on the technical details of masonry veneer and cavity walls - Focused on the out wyth of clay bricks -)

  • 양순갑
    • 한국주거학회논문집
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    • 제8권3호
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    • pp.219-230
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    • 1997
  • Lack of technical standards, specification and inadequate execution in masonry wall construction in Korea lead to produce serious flaw problems such as crack, efflorescene, and upset etc.. The purpose of this paper is to present the practical details for Masonry cavity wall construction to prevent rain penetration and to accommodate differential movement between the inner and outer wythes of cavity walls. Considering rain penetration and differential movement of both wythes of cavity walls, provision of an adequate air space, an airtight back-up wall, clean cavity with weepholes and vents, properly positioned flashing, tie and shelf angle etc. depend on the cavity wall types will help ensure good performance. The present details included noncorrosive hot dip galvanized steel or stainless steel for metal components, plastic and ultra violet resistant polypropylene Copolymer for other components was taken into account the construction method and several types of cavity walls in Korea

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잉크 색상 필터의 광학적 특성 (Optical properties of ink color filters)

  • 이찬구;이수대
    • 한국안광학회지
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    • 제8권1호
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    • pp.23-28
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    • 2003
  • 랩온어칩을 위한 변환 가능한 RGB 색상 필터를 연구하였다. 잉크 색상 필터는 PDMS 패턴과정에 의한 공정으로 제작하였고, 칼라 필터의 자외선-가시광선 영역의 광투과율을 조사하였다. 잉크 칼라 필터는 스펙트럼의 모양과 기울기에 의해 특성 지워진다. 적색/황색 필터의 투과는 600 nm와 500 nm에서 차단스펙트럼 모양을 가지는 곡선으로 구성되었다. 잉크 필터의 청색 출력은 80% 피크 투과율과 약한 적색 누수를 보였다. 한편 녹색 잉크 필터는 48% 피크 투과율과 적색 누수 투과를 보였다.

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Synthesis of $M(WO_4)$:Eu (M : Group 1 or 2) for LED and its Luminescent Properties

  • Park, Seung-Hyok;Kim, Chang-Hae;Park, Hee-Dong;Kim, You-Hyuk
    • 한국정보디스플레이학회:학술대회논문집
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    • 한국정보디스플레이학회 2002년도 International Meeting on Information Display
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    • pp.838-841
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    • 2002
  • $M(WO_4)$:Eu phosphor as a red emitting phosphor for LED was prepared by solid state method. Tungstate phosphors were exited at long wavelength ultra violet region. In special, the emission of Eu-doped $M(WO_4)$:Eu phosphor under the excitation of 410nm appeared at 613nm. $M(WO_4)$:Eu phosphors with M : Group 1 had a higher excitation intensity than those of the phosphors with M: Group 2 at long-wavelength UV.

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PLD증착 변수에 따른 II-VI족 화합물 ZnO 반도체 박막의 발광 특성 연구 (Correlation Between Deposition Parameters and Photoluminescence of ZnO Semiconducting Thin Films by Pulsed laser Deposition)

  • 배상혁;윤일구;서대식;명재민;이상렬
    • 한국전기전자재료학회논문지
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    • 제14권3호
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    • pp.246-250
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    • 2001
  • ZnO thin films for light emission device have been deposited on sapphire and silicon substrates by pulsed laser deposition technique(PLD). A Nd:YAG laser was used with the wavelength of355 nm. In order to investigate the emission properties of ZnO thin films, Pl measurements with an Ar ion laser a light source using an excitation wavelength of 351 nm and a power of 100 mW are used. All spectra were taken at room temperature by using a grating spectrometer and a photomultiplier detector. ZnO exhibited Pl bands centers around 390, 510 and 640 nm, labeled near ultra-violet(UV), green and orange bands. Structural properties of ZnO thin films are analyzed with X-ray diffraction(XRD).

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Vanillylidene imine 유도체의 가수분해 반응에 관한 속도론적 연구 (A study on the Kinetics velocity for hydrolysis reaction of vanillylidene imine derivatives)

  • 성기천;김기준
    • 한국응용과학기술학회지
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    • 제12권2호
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    • pp.145-150
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    • 1995
  • The Kinetics velocity for hydrolysis reaction of vanillylidene imine derivatives has been measured by ultra-violet ray spectrophotometer in 20wt% $dioxane-H_2O$ at $25^{\circ}C$. It was measured the reaction rate Constant of vanillylidene imine derivatives that can be applied widely following to pH-change at $25^{\circ}C$. Final products that hydrolyzed the vanillylidene imine certified in vanillin and aniline derivative, and the effect of substitution radical that has affected on hydrolysis reaction was largely promoted to reaction rate by electron attrating group in acidity and electron donoring group in basic. From the results of rate constant to hydrolysis reaction, substituent radical effect and final products. It has certified the hydrolysis reaction mechanism of vanillylidene imine derivatives.

BRIEF REPORTS ON KAISTSAT-4 MISSION ANALYSIS

  • Seon, J.
    • Journal of Astronomy and Space Sciences
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    • 제17권2호
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    • pp.233-240
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    • 2000
  • Five scientific instruments are planned on KAISTSAT-4 that is scheduled to be launched in 2002. A far ultra-violet imaging spectrograph and a set of space plasma instruments are currently being designed. The imaging spectrograph will make observations of astronomical objects and Earth's upper atmosphere. The plasma instrumentation is capable of fast measuring the thermal magnetosphere plasmas, cold ionospheric plasmas and the Earth's magnetic fields. Major system drivers and constraints on the payloads as well as the spacecraft are identified. A preliminary analysis of the K-4 mission has been undertaken with the system requirements that are derived from the system drivers. Detailed investigation shows that Sun-synchronous orbits with approximate altitudes of 800km are optimal to satisfy the identified requirements. Comparisons with other orbits of different inclinations are also shown. Four operation modes and a daily schedule of spacecraft maneuver are found from the Sun-synchronous orbital model. It is shown that the scientific objectives of K-4 can be achieved with moderate levels of design and operation risks.

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