• 제목/요약/키워드: Gas Radiation

검색결과 620건 처리시간 0.026초

TiO2 광촉매와 UV LED를 이용한 접촉연소식 수소센서 (Catalytic combustion type hydrogen gas sensor using TiO2 and UV LED)

  • 홍대웅;한치환;한상도;곽지혜;이상렬
    • 센서학회지
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    • 제16권1호
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    • pp.7-10
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    • 2007
  • A thick film catalytic gas sensors which can be operated at $142^{\circ}C$ in presence of ultra violet-light emitting diode has been developed to measure hydrogen concentration in 0-5 % range. The sensing material as a combustion catalyst consists of $TiO_{2}$ (5 wt%) and Pd/Pt (20 wt%) supported on $Al_{2}O_{3}$ powder and the reference material to compensate the heat capacity of it in a bridge circuit was an catalyst free $Al_{2}O_{3}$ powder. Platinum heater and sensor materials were formed on the alumina plate by screen printing method and heat treatment. The effect of UV radiation in the presence of photo catalyst $TiO_{2}$ on the sensor sensitivity, response and recovery time has been investigated. The reduction of operating temperature from $192^{\circ}C$ to $142^{\circ}C$ for hydrogen gas sensing property in presence of UV radiation is attributed to the hydroxy radical and superoxide which was formed at the surface of $TiO_{2}$ under UV radiation.

CNG 충전소의 누출$\cdot$확산에 대한 위험성 평가 (The Hazard Assessment of Release and Dispersion of CNG Service Station)

  • 최종운;이수경
    • 한국가스학회지
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    • 제4권3호
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    • pp.53-58
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    • 2000
  • CNG 충전소에 대한 사고영향평가(CA) 분석을 실시하였고 이미 고압법에 의해 설치되어 있는 LPG 충전소에 대한 CA를 실시하여 서로 비교하였다. CNG 충전소와 LPG 충전소에 대한 누출 확산 및 복사열의 영향평가 결과 연소하한계에 도달하는 거리는 CNG 충전소가 LPG 충전소에 비해 약 1.5배 컸으며, 복사열의 경우 공정장치에 손상을 줄 수 있는 복사열량이 CNG 충전소에서는 나타나지 않았으나 LPG 충전소의 경우 37.5 $kw/m^2$에 해당하는 복사열이 12.6 m 반경으로 나타나 주변의 상가지역까지 큰 영향을 미칠 수 있는 것으로 나타났다. 또한, 목재를 태울 수 있을 정도의 복사열량인 12.5 $kw/m^2$은 LPG 충전소가 CNG 충전소에 비해 약 3배 가량 큰 것으로 나타났다.

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개구부가 있는 밀폐공간내 화재의 복합열전달 및 연소가스 분석에 관한 연구 (A Study on the Combined Heat Transfer and Analysis Fire Induced Combustion Gas in a partially Open Enclosure)

  • 박찬국;추병길;김철
    • 한국화재소방학회논문지
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    • 제11권1호
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    • pp.21-35
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    • 1997
  • The natural convection and combined heat transfer induced by fire in a rectangular enclosure is numerically studied. The model for this numerical analysis is partially opened right wall. The solution procedure includes the standard k-$\varepsilon$ model for turbulent flow and the discrete ordinates method (DOM) is used for the calculation of radiative heat transfer equation. In numerical study, SIMPLE algorithm is applied for fluid flow analysis, and the investigations of combustion gas induced by fire is performed by FAST model of HAZARD I program. In this study, numerical simulation on the combined naturnal convection and radiation is carried out in a partial enclosure filled with absorbed-emitted gray media, but is not considered scattering problem. The streamlines, isothermal lines, average radiation intensity and kinetic energy are compared the results of pure convection with those of the combined convection-radiation, the combined heat transfer. Comparing the results of pure convection with those of the combined convection-radiation, the combined heat transfer analysis shows the stronger circulation than those of the pure convection. Three different locations of heat source are considered to observe the effect of heat source location on the heat transfer phenomena. As the results, the circulation and the heat transfer in the left region from heating block are much more influenced than those in the right region. It is also founded that the radiation effect cannot be neglected in analyzing the building in fire. And as the results of combustion gas analysis from FAST model, it is found that O2 concentration is decreased according to time. While CO and CO2 concentration are rapidly increased in the beginning(about 100sec), but slowly decreased from that time on.

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The emission spectrum from isolated black holes

  • Gwon, Sun-Ja;Park, Myeong-Gu
    • 천문학회보
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    • 제40권1호
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    • pp.86.3-86.3
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    • 2015
  • There could be significant numbers of isolated stellar mass black holes in our Galaxy. The detection of these black holes will provide important clues on the origin of supermassive black holes. Interstellar gas will be accreted to these isolated black holes in nearly spherical flow. The gas and the interstellar magnetic field will be compressed and emit bremsstrahlung and magnetic bremsstrahlung. We calculate the density, temperature, magnetic field of the accretion flow onto a 10 solar mass black hole as well as its radiative emission; special attention is given to cyclotron radiation and synchrotron radiation, which covers from microwave to X-ray. We consider the possibility to detect these radiation from isolated Galactic black holes with current instruments and surveys.

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State-of-the-art progress of gaseous radiochemical method for detecting of ionizing radiation

  • Lebedev, S.G.;Yants, V.E.
    • Nuclear Engineering and Technology
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    • 제53권7호
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    • pp.2075-2083
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    • 2021
  • The article provides a review of the research results obtained during of more than 20 years concerning using the gaseous radiochemical method (GRCM) for detecting of ionizing radiation. This method based on threshold nuclear reactions with production of radioactive noble gas which does not interact with the materials of gaseous tract. The applications of GRCM in the diagnostics of neutrinos, neutrons, charged particles, thermonuclear plasma thermometry, and the study of the structure and dynamics of astrophysical objects, position-sensitive dosimetry of neutron targets with accelerator driving, spatial distribution of the fast neutron flux density in a nuclear reactor allowing the transformation of longitudinal coordinate of neutron flux distribution into a temporal distribution of the radiochemical gas decay counting rate ("barcode" semblance) and measurement of bombarding particles spectra are described. Experimental testing of the described technologies was made on the neutron target driven with the linear proton accelerator of Institute for Nuclear Research of Russian Academy of Sciences (INR RAS).

Combined Convection and Radiation in a Tube with Circumferential Fins and Circular Disks

  • Kim, Namjin;Lee, Jaeyong;Taebeom Seo;Kim, Chongbo
    • Journal of Mechanical Science and Technology
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    • 제16권12호
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    • pp.1725-1732
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    • 2002
  • Combined convection and radiation heat transfer in a circular tube with circumferential fins and circular disks is investigated for various operating conditions. Using a finite volume technique for steady laminar flow, the governing equations are solved in order to study the flow and temperature fields. The P- 1 approximation and the weighted sum of gray gases model (WSGGM) are used for solving the radiation transport equation. The results show that the total Nusselt number of combined convection and radiation is higher than that of pure convection. If the temperatures of the combustion gas and the wall in a tube are high, radiation becomes dominant. Therefore, it is necessary to evaluate the effect of radiation on the total heat transfer.

낮은 에너지 감마선과 베타선 모니터링을 위한 Gas Electron Multiplier 검출기의 효율성에 대한 연구 (Research of Efficiency for Gas Electron Multiplier Detector to Monitor Low Energy Gamma-Ray and Beta-Ray)

  • 이순혁;정재훈;이레나
    • 한국의학물리학회지:의학물리
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    • 제25권2호
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    • pp.95-99
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    • 2014
  • 병원을 포함해서서 방사선 물질을 사용하는 모든 사업장에서 방사선 물질의 모니터링은 방사선 안전에 가장 중요한 요소의 하나이다. 본 연구는 방사선 모니터링 시스템에 있어서 GEM 검출기의 활용 가능성을 알아보기 위한 선행 연구로서, GEM 검출기를 제작하고 CdTe 검출기와의 상대적 효율을 구한 결과, 베타와 감마선에 대한 평균 상대 효율이 각각 72%와 4%로서 매우 우수한 성능을 나타냄을 보였다.

Modification of DC Flashover Voltage at High Altitude on the Basis of Molecular Gas Dynamics

  • Liu, Dong-Ming;Guo, Fu-Sheng;Sima, Wen-Xia
    • Journal of Electrical Engineering and Technology
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    • 제10권2호
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    • pp.625-633
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    • 2015
  • The effect of altitude on thermal conduction, surface temperature, and thermal radiation of partial arc was investigated on the basis of molecular gas dynamics to facilitate a deep understanding of the pollution surface discharge mechanism. The DC flashover model was consequently modified at high altitude. The validity of the modified DC flashover model proposed in this paper was proven through a comparison with the results of high-altitude simulation experiments and earlier models. Moreover, the modified model was found to be better than the earlier modified models in terms of forecasting the flashover voltage. Findings indicated that both the thermal conduction coefficient and the surface thermodynamics temperature of partial arc had a linear decrease tendency with the altitude increasing from 0 m to 3000 m, both of which dropped by approximately 30% and 3.6%, respectively. Meanwhile, the heat conduction and the heat radiation of partial arc both had a similar linear decrease of approximately 15%. The maximum error of DC pollution flashover voltage between the calculation value according to the modified model and the experimental value was within 6.6%, and the pollution flashover voltage exhibited a parabola downtrend with increasing of pollution.

Lyα Radiative Transfer and The Wouthuysen-Field effect

  • 선광일;김창구
    • 천문학회보
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    • 제42권2호
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    • pp.43.1-43.1
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    • 2017
  • A three-dimensional (3D) $Ly{\alpha}$ radiative transfer code is developed to study the Wouthuysen-Field effect, which couples the 21 cm spin temperature of neutral hydrogen and the $Ly{\alpha}$ radiation field, and the escape fraction of $Ly{\alpha}$ from galaxies. The Monte Carlo code is capable of treating arbitrary 3D distributions of $Ly{\alpha}$ source, neutral hydrogen and dust densities, gas temperature, and velocity field. It is demonstrated that the resonance-line profile at the center approaches to the Boltzmann distribution with the gas temperature. A plane-parallel ISM model, which is appropriate for the neutral ISM of our Galaxy, is used to calculate the $Ly{\alpha}$ radiation field strength as a function of height above the galactic plane. We also use a two-phase, clumpy medium model which is composed of the cold and warm neutral media (WNM). It is found that the $Ly{\alpha}$ radiation field is strong enough to thermalize the 21 cm spin temperature in the WNM to the gas kinetic temperature. The escape fraction of $Ly{\alpha}$ is found to be a few percent, which is consistent with the $Ly{\alpha}$ observations of our Galaxy and external galaxies.

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An ionization Chamber for a Steel Sheet Thickness Measurement

  • Kim, Han-Soo;Park, Se-Hwa;Kim, Yong-Kyun;Ha, Jang-Ho;Cho, Seung-Yeon
    • Journal of Radiation Protection and Research
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    • 제31권3호
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    • pp.149-153
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    • 2006
  • An ionization chamber is still widely used in many fields by virtue of its' simple operational characteristics and the possibility of its' various shapes. A parallel type of an ionization chamber for a steel sheet thickness measurement was designed and fabricated. High pure xenon gas, which was pressurized up to 6 atm, was chosen as a filling gas to increase the current response and sensitivity for a radiation. A high pressure gas system was also constructed. The active volume and the incident window size of the fabricated ionization chamber were $30\;cm^3\;and\;12\;cm^2$, respectively. Preliminary tests with a 25 mCi $^{241}Am$ gamma-ray source and evaluation tests in a standard X-ray field were performed. The optimal operation voltage was set from the results of the collection efficiency calculation by using an experimental two-voltage method. Linearity for a variation of the steel sheet thickness, which is the most important factor for an application during a steel sheet thickness measurement, was 0.989 in this study.