• 제목/요약/키워드: X-ray spectra

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진단용 X-선 스펙트럼의 몬테칼로 전산모사 측정 (Diagnostic X-ray Spectra Detection by Monte Carlo Simulation)

  • 백철하;이승재;김대홍
    • 한국방사선학회논문지
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    • 제12권3호
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    • pp.289-295
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    • 2018
  • 대부분의 진단용 방사선 장치는 엑스선을 사용하며, 엑스선은 다양한 에너지를 갖는 스펙트럼을 갖는다. 진단 영상에서 엑스선의 정량적 및 정성적 분석은 선량을 줄이면서 영상 화질을 유지하는데 필수적이다. 본 연구의 목적은 진단 영상에 사용되는 엑스선 스펙트럼을 몬테칼로 시뮬레이션으로 측정하는 것이다. 다양한 엑스선 에너지 스펙트럼이 몬테칼로 시뮬레이션으로 측정되었다. 이 스펙트럼들은 다항식을 보간 한 양극 텅스텐 모델에 의해 계산된 결과와 비교하였다. 엑스선 관전압은 50, 60, 80, 100, 110 kV 였다. 검출기로는 카드뮴 텔루라이드와 비정질 셀레늄 물질을 사용하였다. 엑스선 에너지 스펙트럼의 시뮬레이션 결과는 참조 결과와 일치하였고, NRMSD 값은 최소 1.1%에서 최대 5.7%를 보였다. 시뮬레이션 결과에 의하면 진단 영상을 획득할 때 적절한 관전압의 선택을 가능하게 할 것이다. 또한, 영상 획득 전 환자에 전달되는 선량을 예측하는데 기여할 것이다.

A Practical Method to Correct the Saturation Effect in XMCD Spectra

  • Kim, J.Y.
    • Journal of Magnetics
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    • 제13권3호
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    • pp.85-87
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    • 2008
  • I report a simple method to correct the saturation effect in absorption spectra measured in total electron yield (TEY) mode. It does not require additional measurements of the X-ray penetration depth. In order to check the reliability of the method, X-ray magnetic circular dichroism (XMCD) spectra for polycrystalline Fe were measured at two different incident angles, and then processed with the method. The two resultant XMCD spectra were identical, and their sum rule analysis produced the ratios of orbital magnetic moment to spin magnetic moment, which were very close to the well-known value.

Experimental Evaluation of Scattered X-Ray Spectra due to X-Ray Therapeutic and Diagnosis Equipment for Eye Lens Dosimetry of Medical Staff

  • Kowatari, Munehiko;Nagamoto, Keisuke;Nakagami, Koich;Tanimura, Yoshihiko;Moritake, Takashi;Kunugita, Naoki
    • Journal of Radiation Protection and Research
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    • 제47권1호
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    • pp.39-49
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    • 2022
  • Background: For proper monitoring of the eye lens dose, an appropriate calibration factor of a dosimeter and information about the mean energies of X-rays are indispensable. The scattered X-ray energy spectra should be well characterized in medical practices where eye lenses of medical staffs might be high. Materials and Methods: Scattered X-ray energy spectra were experimentally derived for three different types of X-ray diagnostic and therapeutic equipment, i.e., the computed tomography (CT) scan, the angiography and the fluoroscopy. A commercially available CdZnTe (CZT) spectrometer with a lead collimator was employed for the measurement of scattered X-rays, which was performed in the usual manner. Results and Discussion: From the obtained energy spectra, the mean energies of the scattered X-rays lied between 40 and 60 keV. This also agreed with that obtained by the conventional half value layer method. Conclusion: The scattered X-rays to which medical workers may be exposed in the region around the eyes were characterized by means of spectrometry. The obtained mean energies of the scattered X-rays were found to match the flat region of the dosimeter response.

THE X-RAY EMISSION FROM EARLY TYPE GALAXIES

  • Kim, Dong-Woo
    • 천문학논총
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    • 제7권1호
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    • pp.63-69
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    • 1992
  • We have systematically investigated the X-ray spectra of normal galaxies, by using the Imaging Proportional Counter (IPC) data in the Einstein data base. We employed the X-ray color-color plot as well as the standard model fitting method which requires higher signal to noise ratio. We discuss X-ray emission mechanisms in terms of their spectral properties and the signature of cooling flows which are most likely present in X-ray bright early type galaxies. On the average, fits to absorbed thermal spectra show that the X-ray emission temperature of spirals is higher than that of ellipticals. This is consistent with our understanding that accreting binaries are a major X-ray source in spirals, while extended gaseous halos are present in ellipticals. The emission temperature becomes lower with increasing X-ray to optical luminosity ratio in E and S0 galaxies. This result is what we would expect if the emission of X-ray faint early type galaxies consists of a large evolved stellar component, while the gaseous emission becomes dominant in X-ray brighter galaxies. We also find a cool, self-absorbed core in some early type galaxies, which directly indicates the presence of cooling flows in such galaxies.

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투과선량의 수치해석에 의한 전산화단층영상장치 X선의 에너지 분포결정 (Empirical Determination of a CT X-ray Spectra by Numerical Analysis using Transmission Data)

  • 최태진;김옥배;서수지
    • 한국의학물리학회지:의학물리
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    • 제8권2호
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    • pp.35-43
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    • 1997
  • 광자선의 흡수계수교정과 차등 투과력이 관련된 연구에서 X선의 스펙트럼은 중요한 관심사이다. 본 연구에서는 전산화단층영상장치의 80, 120 kVp X선의 실험적 투과선량으로부터 수치해석을 통해 에너지스펙트럼을 구하였다. 투과선량은 직경 30cm, 두께 5mm 내지 92.3 mm의 알루미늄 파이프필터의 중앙에 반도체검출기를 설치하고 10mm 슬릿빔의 투과선량을 측정하였다. 스펙트럼재구성은 텅스텐타켓의 특성 X선을 포함한 반복적 수치 해석을 통해 에너지 구간별 스펙트럼을 구하였으며 에너지구간은 2keV로 하였다. 재구성한 에너지분포를 이용하여 계산된 투과선량과 측정투과선량의 비교는 두 광자에너지에서 모두 좋은 일치를 보였다. 에너지구간별 분할조사선량의 반복적 계산에 근거를 둔 수치해석은 흡수체의 감쇄된 선속으로부터 X선의 에너지스펙트럼을 매우 유용하게 결정할 수 있음을 보여주었다.

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ISO Narrow Series및 ANSI의 X선 스펙트럼, 평균에너지 및 선량환산인자의 이론적 계산 (Calculations of ISO Narrow and ANSI X-Ray Spectra, Their Average Energies and Conversion Coefficients)

  • 김장렬;김봉환;장시영;이재기
    • Journal of Radiation Protection and Research
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    • 제20권2호
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    • pp.129-136
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    • 1995
  • 중저준위 에너지 범위에서 방사선관리용측정기기의 에너지의존성에 대한 연구를 위하여 ISO에서 는 ISO표준 X선장을 발간하였으며, 또한 ANSI에서도 개인방사선측정 기기의 성능시험을 위하여 ANSI X선장을 제시 하였다. 그러나 X선 스펙트럼의 측정은 많은 시간이 소요될 뿐만 아니라 특히 측정 X선 스펙트럼에 unfolding이 수행된다면 매우 어려운 작업이 된다. 따라서 이론적인 방법에 의해 스펙트럼을 계산 예측하고 그 평균에너지 및 선량환산인자를 계산하는 것은 X선 실험제작에 필요한 시간, 노력 및 비용을 최소화 할 수 있을 것이다. 따라서 본 연구에서는 ISO Narrow series 및 ANSI X선장에 대하여 이론적으로 스펙트럼을 계산하였으며, 그에 의한 평균에너지와 선량당량혼산인자를 계산하였다. 본 계산에 의한 평균에너지 및 선량환산인자는 측정스펙트럼에 의한 ISO 및 X선장의 값과 잘 일치하였다.

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X-선 스펙트럼 변조 기술 연구 (X-Ray Spectrum Modulation for Mammography)

  • 김광현;김경락;오창현
    • 대한전기학회:학술대회논문집
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    • 대한전기학회 2003년도 학술회의 논문집 정보 및 제어부문 B
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    • pp.600-603
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    • 2003
  • Energy spectrum modulation of X-ray source in digital mammography has been studied. In this study, we calculated various filtered spectra using the scattering data. Primary spectra were generated by Molybdenum (Mo) and Tungsten (W) targets. The materials of added filters are Molybdenum and Rhodium (Rh) for 40 kVp Mo. primary spectrum, the amounts of photons over whole energy ranges are attenuated to 0.43 with 0.03 mm Mo filter and 0.38 with 0.06 mm Mo filter while the photons of energy ranged from 17 keV to 20 keV. The photons of low energy ranged below 17 keV are considerably attenuated. This effect brings out reducing the scattered radiation and dose to the patient, and enhancing subject contrast in the image. The results show that filtered spectra are not seriously affected by X-ray tube loadability. Because the energy range from 17 keV to 20 keV is directly transmitted although low and high energies are mainly filtered.

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Calculation of X-ray spectra characteristics and kerma to personal dose equivalent Hp(10) conversion coefficients: Experimental approach and Monte Carlo modeling

  • Arectout, A.;Zidouh, I.;Sadeq, Y.;Azougagh, M.;Maroufi, B.;Chakir, E.;Boukhal, H.
    • Nuclear Engineering and Technology
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    • 제54권1호
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    • pp.301-309
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    • 2022
  • This work aims to establish some X-ray qualities recommended by the International Standard Organization (ISO) using the half-value layer (HVL) and Hp(10) dosimetry approaches. The HVL values of the following qualities N-60, N-80, N-100, N-150 and N-250 were determined using various attenuation layers. The obtained results were compared to those of reference X-ray beam qualities and a good agreement was found (difference less than 5% for all qualities). The GAMOS (Geant4-based Architecture for Medicine-Oriented Simulations) radiation transport Monte Carlo toolkit was employed to simulate the production of X-ray spectra. The characteristics HVLs, mean energy and the spectral resolution of simulated spectra have been calculated and turned out to be conform to the ISO reference ones (difference less than the limit allowed by ISO). Furthermore, the conversion coefficients from air kerma to personal dose equivalent for simulated and measured spectra were fairly similar (the maximum difference less than 4.2%).

A Practical Method for Estimating High-Energy X-Ray Spectra Using the Iterative Perturbation Principle of Waggener

  • Iwasaki, Akira;Matsutani, Hideya;Kubota, Mamoru;Fujimori, Akira;Suzaki, Katsumasa;Abe, Yoshinao
    • 한국의학물리학회:학술대회논문집
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    • 한국의학물리학회 2002년도 Proceedings
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    • pp.263-266
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    • 2002
  • We have developed a practical method for estimating high-energy x-ray spectra using measured attenuation curves. This method is based on the iterative perturbation technique proposed by Waggener et al. The principle is to minimize the difference between the measured and calculated transmission curves. The experimental study was made using 4 MV, 10 MV, and 15 MV x-ray beams. It has been found that the spectrum varies strongly with the off-axis distance.

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