• 제목/요약/키워드: Scattering Center

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PET/CT실에서 사용되는 주사기 차폐체의 산란선 측정 (Scattering Measurement of Syringe Shield Used in PET/CT)

  • 장동근;박철우;박은태
    • 대한방사선기술학회지:방사선기술과학
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    • 제43권5호
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    • pp.375-382
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    • 2020
  • PET/CT is a medical equipment that detects 0.511 MeV of gamma rays. The radiation workers are inevitably exposed to ionizing radiation in the process of handling the isotope. Accordingly, PET/CT workers use syringe shields made of lead and tungsten to protect their hands. However, lead and tungsten are known to generate very high scattering particles by interacting with gamma rays. Therefore, in this study, we tried to find out the effect on the scattering particles emitted from the syringe shield. In the experiment, first, the exposure dose to the hand (Rod phantom) was evaluated according to the metal material (lead, tungsten, iron, stainless steel) using Monte Carlo simulation. The exposure dose was compared according to whether or not plastic is attached. Second, the exposure dose of scattering particles was measured using a dosimeter and lead. As a result of the experiment, the shielding rate of plastics using the Monte Carlo simulation showed the largest difference in dose of about 40 % in lead, and the lowest in iron, about 15 %. As a result of the dosimeter test, when the plastic tape was wound on lead, it was found that the reduction rate was about 15 %, 28 %, and 39 % depending on the thickness. Based on the above results, it was found that 0.511 MeV of gamma ray interacts with the shielding tool to emit scattered rays and has a very large effect on radiation exposure. However, it was considered that the scattering particles could be sufficiently removed with plastics with a low atomic number. From now on, when using high-energy radiation, the shielding tool and the skin should not be in direct contact, and should be covered with a material with a low atomic number.

An Analysis of Inelastic Neutron Scattering by Liquid Methane

  • Chung, Chang-Hyun;Shin, Won-Kee;Kim, Jin-Soo
    • Nuclear Engineering and Technology
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    • 제5권4호
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    • pp.265-278
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    • 1973
  • 분자의 병진운동과 회전운동의 상관함수에 대한 감쇠함수 모델을 사용하여 분자액체의 비간섭중성자 산란단면적을 분석하였다. 이러한 방법은 직접적으로 산란함수를 구한다는 점에서 중간함수를 거치는 종래의 방법과는 판연히 다르다. 감쇠함수는 그장파장극한과 일반진동수 분포함수간의 간단한 관계에서 결정하였고 병진운동과회전 운동의 결합관계는 무시된다고 가정하였다. 분자질량중심의 병진운동은 그 짧은 시간과 장시간에서의 행위를 적절히 기술하는 물리적 모텔을 사용하였고 회전운동은 쌍극상관함수 또는 적외선진동 홈수스펙트럼의 푸리어 변환으로 된 감쇠함수에 관계된다고 가정하였다. 액체메탄에 대한 이론적 절대 산란강도를 계산하였으며 이는 열 및 냉중성자 측정치와 만족할만한 일치를 보여주고 있다.

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Effect of Titanium Nanorods in the Photoelectrode on the Efficiency of Dye Sensitized Solar Cells

  • Rahman, Md. Mahbubur;Kim, Hyun-Yong;Jeon, Young-Deok;Jung, In-Soo;Noh, Kwang-Mo;Lee, Jae-Joon
    • Bulletin of the Korean Chemical Society
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    • 제34권9호
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    • pp.2765-2768
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    • 2013
  • The effect of $TiO_2$ nanorods (TNR) and nanoparticles (TNP) composite photoelectrodes and the role of TNR to enhance the energy conversion efficiency in dye-sensitized solar cells (DSSCs) was investigated. The 5% TNR content into the TNP photoelectrode significantly increased the short-circuit current density ($J_{sc}$) and the open-circuit potential ($V_{oc}$) with the overall energy conversion efficiency enhancement of 13.6% compared to the pure TNP photoelectrode. From the photochemical and impedemetric analysis, the increased $J_{sc}$ and $V_{oc}$ for the 5% TNR/TNP composite photoelectrode was attributed to the scattering effect of TNR, reduced electron diffusion path and the suppression of charge recombination between the composite photoelectrode and electrolyte or dye.

Aerosol radiative forcing estimated from ground-based sky radiation measurements over East Asia

  • Kim, Do-Hyeong;Sohn, B.J.;Nakajima, T.;Okada, I.;Takamura, T.
    • 대한원격탐사학회:학술대회논문집
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    • 대한원격탐사학회 2002년도 Proceedings of International Symposium on Remote Sensing
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    • pp.12-16
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    • 2002
  • The clear sky radiative forcings of aerosols were evaluated over East Asia. We first investigated optical characteristics of aerosol using sky radiation measurements. An algorithm of Nakajima et al. (1996) is used for retrieving aerosol parameters such as optical thickness, ${\AA}$ngstr$\"{O}$m exponent, single scattering albedo, and size distribution from sky-radiation measurements, which then can be used for examining spatial and temporal variations of aerosol. Obtaining aerosol radiative forcing at TOA and surface, a radiative transfer model is used with inputs of obtained aerosol parameters and GMS-5 satellite-based cloud optical properties. Results show that there is a good agreement of simulated downwelling radiative flux at the surface with observation within 10 W m$^{-2}$ rms errors under the clear sky condition. However, a relatively large difference up to 40 W m$^{-2}$ rms error is found under the cloudy sky condition. The computed aerosol radiative forcing at the surface shows downward flux changes ranging from -100 to -170 W m$^{-2}$ per unit aerosol optical thickness at 0.7 $\mu$m. The different values of aerosol radiative forcing among the stations is mainly due to the differences in single scattering albedo ($\omega$$_{0.7}$) and asymmetric parameter (g$_1$) related to the geographical and seasonal variations.

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수중음향 모델을 위한 보름달물해파리(Aurelia aurita s.l.)의 체내 음속비 및 밀도비 (Measurements of Sound Speed and Density Contrasts of the Moon Jellyfish (Aurelia aurita s.l.) for Hydroacoustic Model)

  • 강돈혁;이창원;이형빈;김미라
    • Ocean and Polar Research
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    • 제34권1호
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    • pp.85-91
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    • 2012
  • Physical properties such as sound speed contrast (h) and density contrast (g) of the interested target are key parameters to understand acoustic characteristics by using theoretical scattering models. The density and sound speed of moon jellyfish (common jellyfish, Aurelia aurita s.l.) were measured. Sound speed contrast (h) was measured from travel time difference (time-of-flight method) of an acoustic signal in a water tank for APOP studies (Acoustic Properties Of zooplankton). Density contrast (g) was measured by the displacement volume and wet weight (dual-density method). The sound speed remained almost constant as the moon jellyfish increased in bell length. The mean values${\pm}$standard deviation of h and g were $1.0005{\pm}0.0012$ and $0.9808{\pm}0.0195$), respectively. These results will provide important input for use in theoretical scattering models for estimating the acoustic target strength of jellyfish.

(고분자/액정) 복합막의 상분리구조와 전기광학 특성 (Phase Separated Structure and Electro-optical Properties of the (Polymer/Liquid Crystal) Composite Films)

  • 박관선;노창호;사공동식;남기대;카지야마
    • 한국응용과학기술학회지
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    • 제12권2호
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    • pp.29-39
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    • 1995
  • The phase separated structure and the electro-optical properties of the (polymer/liquid) crystal : LC) composite film strongly depended on the weight fraction of LC in it. The continuous LC phase was formed in a three-dimensional polymer network when the LC weight fraction was above 40wt%. The aggregation structure of the composite film could be controlled by controlling the solvent evaporation velocity during the film preparation process. The smaller LC domains or channels were formed in the case of the faster solvent evaporation velocity. The composite film exhibited reversible light scattering-light transmission switching upon electric field -OFF and -ON states, respectiverly. The light scattering properties of the composite film strongly depended on the spatial distortion of the nematic directors as well as the mismatch in refractive indices between matrix polymer and LC.

EFFECTS OF COLLISIONAL DE-EXCITATION ON THE RESONANCE DOUBLET FLUX RATIOS IN SYMBIOTIC STARS AND PLANETARY NEBULAE

  • Kang, Eun-Ha;Lee, Hee-Won
    • 천문학회지
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    • 제41권3호
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    • pp.49-58
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    • 2008
  • Resonance doublets including O VI 1032, 1038, NV 1239, 1243 and C IV 1548, 1551 constitute prominent emission lines in symbiotic stars and planetary nebulae. Spectroscopic studies of symbiotic stars and planetary nebulae from UV space telescopes show various line ratios of these doublets deviating from the theoretical ratio of 2:1. Using a Monte Carlo technique, we investigate the collisional de-excitation effect in these emission nebulae. We consider an emission nebula around the hot component of a symbiotic star characterized by the collisional de-excitation probability $p_{coll}\;{\sim}\;10^{-3}\;-\;10^{-4}$ per each resonance scattering, and the line center optical depths for major resonance doublets in the range ${\tau}_0\;{\sim}\;10^2\;-\;10^5$. We find that various line ratios are obtained when the product $p_{coll}{\tau}_0$ is of order unity. Our Monte Carlo calculations show that the flux ratio can be approximately fitted by a linear function of ${\log}{\tau}_0$ when ${\tau}_0p_{coll}\;{\sim}\;1$. It is briefly discussed that this corresponds to the range relevant to the emission nebulae of symbiotic stars.

Characterization of Poly(vinyl phosphate-b-styrene) by Solid-State $^{31}P$ NMR and Titration

  • Li, Guang-Hua;Kim, Sang-Hun;Cho, Chang-Gi;Park, Tae-Joon;Kim, Yong-Ae
    • Macromolecular Research
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    • 제14권5호
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    • pp.504-509
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    • 2006
  • Poly(vinyl phosphate-b-styrene) (PVPP-b-PS) block copolymers were synthesized successfully from poly(vinyl alcohol-b-styrene) (PVA-b-PS) by reaction with phosphorus oxychloride and subsequent hydrolysis. The obtained block copolymers were slightly crosslinked, and were characterized by various analytical techniques. The total phosphorus content and the ratio of the differently bound phosphorus were obtained by both solid-state $^{31}P$ NMR and pH titration, but the results differed slightly. Characterization by energy dispersion X-ray analysis (EDS) or Rutherford back scattering (RBS), on the other hand, determined the total phosphorus contents, but the results were quite different from those by solid-state $^{31}P$ NMR.