• Title/Summary/Keyword: Ionized gas

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Deposition of Indium Tin Oxide films on Polycarbonate substrates by Ion-Assisted deposition (IAD)

  • Cho, Jn-sik;Han, Young-Gun;Park, Sung-Chang;Yoon, Ki-Hyun;Koh, Seok-Keun
    • Proceedings of the Korean Vacuum Society Conference
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    • 1999.07a
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    • pp.98-98
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    • 1999
  • Highly transparent and conducting tin-doped indium oxide (ITO) films were deposited on polycarbonate substrate by ion-assited deposition. Low substrate temperature (<10$0^{\circ}C$) was maintained during deposition to prevent the polycarbonate substrate from be deformed. The influence of ion beam energy, ion current density, and tin doping, on the structural, electrical and optical properties of deposited films was investigated. Indium oxide and tin-doped indium oxide (9 wt% SnO2) sources were evaporated with assisting ionized oxygen in high vacuum chamber at a pressure of 2$\times$10-5 torr and deposition temperature was varied from room temperature to 10$0^{\circ}C$. Oxygen gas was ionized and accelerated by cold hallow-cathode type ion gun at oxygen flow rate of 1 sccm(ml/min). Ion bea potential and ion current of oxygen ions was changed from 0 to 700 V and from 0.54 to 1.62 $\mu$A. The change of microstructure of deposited films was examined by XRD and SEM. The electrical resistivity and optical transmittance were measured by four-point porbe and conventional spectrophotometer. From the results of spectrophotometer, both the refractive index and the extinction coefficient were derived.

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Electrical Breakdown In flames

  • Uhm, Han S.
    • Journal of Korean Vacuum Science & Technology
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    • v.4 no.1
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    • pp.33-37
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    • 2000
  • Properties of electrical discharge in flames and influence of plasma electrons on gas neutrals are investigated by making use of the ionization cross section of air. Frames have three distinctive features. They are hot, emit light and are weakly ionized. We investigate influence of these three characteristics of flames on the electrical breakdown. It is found that the breakdown electric field in flames is inversely proportional to the flame temperature T$\_$g/, thereby easily generating plasmas in flames. A swarm of low-energy electrons in flames would allow a significant population of electronically excited states of flame molecules to be formed. Therefore, the analysis shows that the electronic excitation of flame molecules may also considerably reduce the breakdown field. Plasma electrons generate atomic oxygen by the electron attachment of oxygen molecules in high-pressure flames. These oxygen atoms are the most reactive radicals in flames for material oxidation.

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Kinetics of $CO_2$ Absorption in Aqueous AMP (2-amino-2-methyl -1-propanol) Solutions

  • Park, Moon-Ki
    • Environmental Sciences Bulletin of The Korean Environmental Sciences Society
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    • v.2 no.1
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    • pp.85-90
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    • 1998
  • The reaction rate of $CO_2$ with 2-amino-2-methyl-1-propanol (AMP), MEA monoethanolamine(MEA) and diethanolamine (DEA) in aqueous solutions has been determined using a stirred vessel with a plane gas-liquid interface over a wide range of concentrations of amines at different temperatures. The results show that the overall reaction rate is first order with respect to both $CO_2$ and amine. The reaction rate constant varies with temperature according to the relationship which agrees with the experimental data. The proposed interpretation is that the kinetic rate determining step is a reaction of $CO_2$ with amine to form carbamic acid which is then totally and immediately ionized.

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Infrared Study of a Low-mass Star-forming Region L1251B

  • Choi, Yunhee;Lee, Jeong-Eun;Bergin, Edwin A.;Blake, Geoffrey A.;Boogert, A.C. Adwin;Francesco, James Di;Evans, Neal J. II;Pontoppidan, Klaus M.;Sargent, Annelia I.
    • The Bulletin of The Korean Astronomical Society
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    • v.41 no.2
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    • pp.56.1-56.1
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    • 2016
  • A low-mass star-forming region, L1251B, is an excellent example of a small and nearby group of protostellar objects. L1251B has been mapped spectroscopically with the Infrared Spectrograph (IRS) onboard the Spitzer Space Telescope. IRS has provided mid-IR emission lines (e.g., [Fe II], [Ne II], and ro-vibrational H2) and absorption features of CO2 and H2O ice in studying the physical state of the ionized gas and the material residing in the circumstellar environments. We will present the distribution of outflows and ice components in L1251B.

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Synthesis of ZnO nanowires and their optical characteristic properties (ZnO 나노와이어의 합성 및 광학적 특성)

  • 박광수;이종수;강명일;김항성;성만영;김상식
    • Proceedings of the Korean Institute of Electrical and Electronic Material Engineers Conference
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    • 2002.07a
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    • pp.43-49
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    • 2002
  • Gray-colored materials were synthesized from ball-milled ZnO powders under a thermal annealing at 1380$^{\circ}C$ with an argon carrier gas for 3 hours. The synthesized materials were identified to be wurtzitic hexagonal structured ZnO nanowires by X-ray diffraction and scanning electron microscopy. The ZnO nanowires have the long cylinder-like shape of which cross-section is a circle, and these nanowires are in the range 15∼40 nm width and 10-70 $\mu\textrm{m}$ length, respectively. Transmission electron microscopy revealed that these nanowires are single-crystalline and grow along [110] direction. The optical properties of the ZnO nanowires were investigated with photoluminescence. The analytic results revealed that ZnO nanowires have the singly ionized oxygen vacancies in the surface lattices, as they emit strong green light in room temperature PL. In addition, the growth mechanism of the ZnO nanowires can be described by the vapor-solid procedures.

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A study on the electrical characteristics and the growth of $Al_ 2O_3$ film on Si with low temperatures by GAIVBE technique (GAIVBE기법에 의한 저온 $Al_ 2O_3$ on Si 박막의 형성과 전기적 특성에 관한 연구)

  • ;;;K.V.Rao
    • Electrical & Electronic Materials
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    • v.8 no.3
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    • pp.306-315
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    • 1995
  • 본 논문에서는 $Al_{2}$ $O_{3}$박막을 GAIVBE(Gas Assisted Ionized Vapour Beam Epitaxy)기법에 의해 저온에서 300-1,400.angs.의 두께로 성장하여 그 조건을 제시하였다. 아울러 Al-Al$_{2}$ $O_{3}$-Si의 MOS구조를 제작하여 전기적 특성을 고찰하고 그 결과를 분석, 제시하므로써 GAIVBE기법에 의해 저온으로 형성된 $Al_{2}$ $O_{3}$막의 활용 가능성을 보고하였다. 한편, 본 연구에서 제작한 $Al_{2}$ $O_{3}$막의 저항율은 막의 두께 100-1,000.angs.인 시료제작에서 $10^{8}$ohm-cm 와 $10^{13}$ohm-cm로 측정되었고, 비유전율은 9.5-10.5, 절연파괴강도 6-7MV/cm(+바이어스)와 11-12MV/cm(-바이어스)이었다.

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Synthesis of ZnO Nanowires and their Characteristic Properties (ZnO 나노와이어의 합성 및 특성)

  • 박광수;이종수;강명일;성만영;김상식
    • Journal of the Korean Institute of Electrical and Electronic Material Engineers
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    • v.15 no.8
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    • pp.651-657
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    • 2002
  • Gray-colored materials were synthesized from ball-milled ZnO powders under a thermal annealing at $1380^{\circ}C$ with an argon carrier gas for 3 hours. The synthesized materials were identified to be wurtzitic hexagonal structured ZnO nanowires by X-ray diffraction and scanning electron microscopy. The ZnO nanowires have the long cylinder-like shape of which cross-section is a circle, and these nanowires are in the range 15~40nm width and 10~70 $\mu m$ length, respectively. Transmission electron microscopy revealed that these nanowires are single-crystalline and grow along [110] direction. The optical properties of the ZnO nanowires were investigated with photoluminescence. The analytic results revealed that ZnO nanowires have the singly ionized oxygen vacancies in the surface lattices, as they emit strong green light in room temperature PL. In addition, the growth mechanism of the ZnO nanowires can be described by the vapor-solid procedures.

EMISSION LINE VELOCITY FIELD OF THE MAGELLANIC IRREGULAR GALAXY NGC 4449

  • SASAKI MINORU;OHTANI HIROSHI;SAITO MAMORU;OHTA KOUJI;YOSHIDA MICHITOSHI;SHIMIZU TASUHlRO;KOYANO HISASHI;KOSUGI GEORGE;AOKI KENTARO;SASAKI TOSHIYUKI
    • Journal of The Korean Astronomical Society
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    • v.29 no.spc1
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    • pp.85-86
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    • 1996
  • The imaging spectroscopic observations of the Magellanic irregular galaxy NGC 4449 were made to show the detailed kinematic structure of the galaxy. Many filamentary structures and Several bubble-like structures are recognized in a 3D data cube of H$\alpha$ emission line. Velocity field shows the kpc-scale mosaic structure and counter- rotation of ionized gas.

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Narrow-line Region of Type I QSOs

  • Oh, Se-Myeong;Woo, Jong-Hak;Bennert, Vardha
    • The Bulletin of The Korean Astronomical Society
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    • v.36 no.2
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    • pp.62.1-62.1
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    • 2011
  • We investigate various physical parameters of the narrow-line region (NLR) of two type I QSOs, PG1012+008 and PG1307+085. Using the spectra obtained with the FORS1 at the VLT with an excellent seeing condition (<0.7"), we can extract spectra with varying distances from the center out to the galactic scales. From these spectra we derive physical quantities such as reddening, temperature, electron density, and ionization parameter as a function of distance from the center. We also explore the possibility of defining the size of the NLR with line ratio diagnostics regardless of starbursts, shock-ionized gas, or tidal tails.

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Electrical and Optical Properties of Microwave Discharged Lamp (마이크로파 방전램프의 전기적/광학적 특성)

  • Lee, Jong-Chan;Hwang, Myung-Keun;Bae, Young-Jin;Her, Hyun-Soo;Park, Dae-Hee
    • Proceedings of the Korean Institute of Electrical and Electronic Material Engineers Conference
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    • 2002.11a
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    • pp.492-494
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    • 2002
  • The fundamental principles of the operation of microwave discharges that are used to convert microwave energy to broad spectrum visual light are known. In this paper, emission dependance of microwave discharges in mixture content of sulfur with noble gases was studied. It is shown that the excitation of this gaseous mixture is carried out in two phases: (1) ionization of noble gas atoms by a microwave field and (2) the consequent maintenance of slightly ionized nonequilibrium plasma by the field. These two processes have essentially various thresholds for the microwave pump. The purpose of this work is to investigate spectral properties of the high frequency discharges in a mixture sulfur vapors with noble gases.

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