• Title/Summary/Keyword: Radiation and Scattering

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Fast Converging Correction Current for the Physical Optics Edge Diffraction by a dielectric Wedge (유전체 쐐기에 의한 물리광학해를 수정하기 위한 새 로운 급수)

  • 전재영;서종화;나정웅
    • Proceedings of the IEEK Conference
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    • 1999.06a
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    • pp.877-880
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    • 1999
  • A rigorous formulation is suggested〔l,2,3〕 in solving the scattering of plane waves by a dielectric wedge. Correcting surface currents are expanded in a Neumann series of fractional orders to meet the edge condition of static limit〔4〕. For the better converging series, the modified Neumann series satisfying the static limit edge condition and the radiation condition are suggested here for the surface currents having two different wave numbers of air and dielectric〔4〕. This representation gives accurate solutions over the whole region including the grazing incidence of the plane waves upon the dielectric wedge of large permittivities.

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Electromagnetic Wave Scattering from Multilayered Circular Cylinder : OSRC Approach (다층고조를 갖는 원형 실린더에 의한 전자파 산란 : OSRC 방법)

  • 이화춘;이대형;최병하
    • Journal of the Korean Institute of Telematics and Electronics A
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    • v.32A no.3
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    • pp.38-44
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    • 1995
  • The scattered electric field from a multilayered circular dielectric cylinder is caculated. Approximate boundary condition used in on-surface radiation boundary condition(OSRC) method has been applied to all the boundary surface of N-layered dielectric cylinder. It was assumed that scattered electric field at inner boundary surface in one region transmitted to the adjacent region at outer boundary surface. In the whole region, the unknown coefficients of electric field are acquired by the given incident electric field with ease. Electric field distribution at each boundary surface and the scattered electric field in free space are taken with the calculated unknown coefficients. the results obtainted were compared with those results that were used by regular surface boundary condition.

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Advanced Analysis Techniques for Oxide Cathodes

  • Je, Jung-Ho;Kim, In-Woo;Seol, Seung-Kwon;Kwon, Yong-Bum;Cho, Chang-Sik;Weon, Byung-Mook;Park, Gong-Seog;Hwang, Cheol-Ho;Hwu, Yeukuang;Tsai, Wen-Li
    • 한국정보디스플레이학회:학술대회논문집
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    • 2003.07a
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    • pp.1155-1156
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    • 2003
  • The advanced analysis techniques such as high resolution X-ray absorption spectroscopy (XAS), X-ray scattering, and photoelectron emission microscope (PEEM) using synchrotron radiation are probably able to open new opportunities for improving the performances of oxide cathodes with more clear and deep understanding.

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A Study on the Radiation Heat Transfer Characteristics of Liquid Droplet Radiator (액적방열기의 복사열전달 특성에 관한 연구)

  • 김금무;김용모;김경근
    • Journal of Advanced Marine Engineering and Technology
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    • v.18 no.1
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    • pp.32-40
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    • 1994
  • The radiative heat transfer analysis in particle layer has an inherent difficulty in treating the governing integro-differential equations, which are derived from the remote effects. Most of the existing analyses are limited to the one dimensional system, taking into account only absorption or isotropic scatting of solid particles. Fortunately, a new Monte Carlo Simulation method is recently developed to analyse multidimensional radiative heat transfer in particles with anisotropically scatting. By this method, the present study analyses the radiative heat transfer in dispersed particles through the numerous droplets in the liquid droplet radiator to develop a technique of liquid droplet radiator. Consequently, knows that the radiative heat flux in particle layer is influenced by exitinction coefficient, optical thickness and surface area of particles in the system.

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A Study on Ultrasonic Testing Simulation using the Multi-Gaussian Beam Model (다중-가우시안 빔 모델을 이용한 초음파 탐상 시험 시뮬레이션에 관한 연구)

  • Song, Sung-Jin;Kim, Hak-Joon
    • Proceedings of the KSME Conference
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    • 2001.06a
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    • pp.553-560
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    • 2001
  • Recently, ultrasonic testing simulation has becomes very important in the field of nondestructive evaluation due to its unique capability of providing testing signals without real inspection. The ultrasonic testing simulation requires three elementary models including the transducer beam radiation model, the flaw scattering model, and the reception model. In the present work, we briefly describe an approach to develop the ultrasonic testing model together with its elementary models with the multi-gaussian beam model. Based on this approach, we developed ultrasonic testing simulation program with MATLAB. The performance of the developed program is demonstrated by the predicting of ultrasonic signals from two types of flaws, circulars crack and spheres.

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The study of oxygen molecules on Pt (111) surface with high resolution x-ray photoemission spectroscopy

  • Kim, Yong-Su;Bostwick, Aaron;Rotenberg, Eli;Ross, Philip N.;Hong, Soon-Cheol;Mun, Bong-Jin Simon
    • Proceedings of the Korean Vacuum Society Conference
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    • 2010.08a
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    • pp.61-61
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    • 2010
  • By using high resolution x-ray photoelectron spectroscopy, we show that inelastic scattering of photoelectron at low temperature (30K~50K) generates two kinds of oxygen species on Pt (111) surface. Intense synchrotron radiation source dissociates oxygen molecules into chemisorbed atomic oxygen and induces the formation of PtO on surface. Estimated coverage of dissociated atomic oxygen is 0.5 ML, suggesting possible formation of p($2{\times}1$) surface structure, while PtO coverage shows saturation coverage of 0.5 ML. Molecular oxygen dosed at 30 K undergoes thermally activated transition from physisorbed to chemisorbed state at around 40K.

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Features in broadband SEDs of young pulsar wind nebulae: existence of two different electron populations

  • Kim, Chanho;An, Hongjun
    • The Bulletin of The Korean Astronomical Society
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    • v.46 no.2
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    • pp.51.2-52
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    • 2021
  • Pulsar Wind Nebula(PWN)는 radio부터 TeV band까지 넓은 파장에 걸쳐 복사를 하며 이 복사는 Spectral Energy Distribution(SED)으로 측정된다. 관측된 SED는 두 개의 주요한 bump를 보이는데 low-energy emission bump는 synchrotron radiation에 의해 만들어지고 high-energy emission bump는 inverse Compton scattering에 의해 만들어진다. 대부분 PWN들의 SED는 단일 전자 분포로 설명이 가능하지만 최근 연구 결과에 의하면 Crab nebula, G21.5-0.9 같은 일부 young pulsar wind nebula의 X-ray SED에서 단차나 기울기의 변화 등 단일 전자 분포로 설명하기 어려운 부분이 관측되기도 한다. 이런 PWN에 대하여 우리는 이중 전자 분포를 이용해서 broadband SED가 잘 설명이 되는지 확인하고 이를 통하여 PWN 입자 가속의 특성을 이해해보고자 한다.

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Evaluation of Abrasive Wear Face Using SAW (표면탄성파를 이용한 마모 표면부의 평가)

  • Kwon, Sung-D.;Yoon, Seok-S.;Song, Sung-J.;Lee, Young-Z.
    • Journal of the Korean Society for Nondestructive Testing
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    • v.22 no.2
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    • pp.193-197
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    • 2002
  • The frequency dependency of the Rayleigh surface wave was investigated indirectly by measuring the angular dependency of the backward radiation of the incident ultrasonic wave in the abrasion specimens, which was explained in view of the residual stress distribution. The peak intensity of the backward radiation profile decreased and the right half width of the profile increased with an increase of the variational rate of residual stress for the scuffing specimen. The peak intensity was also affected by the surface wave scattering during the propagation around the micro-damages. The peak angle might depend on not only the amount of residual stress but also the micro-structure. The result observed in this study demonstrates the high potential of the backward radiated ultrasound as a tool for the nondestructive evaluation of the subsurface gradients of materials.

Line-profile Formula in the Carbon Nanotubes by Electron Spin Resonance

  • Park, Jung-Il;Lee, Haeng-Ki
    • Journal of the Korean Magnetic Resonance Society
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    • v.16 no.1
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    • pp.11-21
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    • 2012
  • The line-width of carbon nanotubes (CNTs) was studied as a function of the temperature at a frequency of 9.49 GHz in the presence of external electromagnetic radiation. The relative frequency dependence of the absorption power is obtained with the projection operator technique (POT) proposed by Kawabata. The line-width increased as the temperature increased in the high-temperature region (T>200 K). The scattering is little affected in the low-temperature region (T<200 K) because there is no correlation between the resonance field and the Fermi-Dirac distribution function. Thus, the present technique is considered to be more convenient to explain the resonant system as in the case of other optical transition problems.

PRIMORDIAL BLACKHOLE AS A SEED FOR THE COSMIC MAGNETIC FIELD

  • LA DAIL;PARK CHANGBOM
    • Journal of The Korean Astronomical Society
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    • v.29 no.2
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    • pp.83-91
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    • 1996
  • We present a model that rotating primordial blackholes(PBHs) produced at the end of inflation generate the random, non-oriented primordial magnetic field. PBHs are copiously produced as the Universe completes the cosmic phase transition via bubble nucleation and tunneling processes in the extended inflation hypothesis. The PBHs produced acquire angular momentum through the mutual tidal gravitational interaction. For PBHs of mass less than 1013g, one can show that the evaporation (photon) luminosity of PBHs exceeds the Eddington limit. Thus throughout the lifetime of the rotating PBH, radiation flow from the central blackhole along the Kerr-geodesic exerts torque to ambient plasma. In the process similar to the Bierman's battery mechanism electron current reaching up to the horizon scale is induced. For PBHs of Grand Unified Theories extended inflation with the symmetry breaking temperature of $T_{GUT}\;\~\;10^{10}$ GeV, which evaporate near decoupling, we find that they generate random, non-oriented magnetic fields of $\~10^{-11}G$ on the last-scattering surface on (the present comoving) scales of $\~O(10)Mpc$.

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