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Background Reduction of Cosmic X-ray Detector By Means of High Speed Pulse Shape Processing

Background Reduction of Cosmic X-ray Detector By Means of High Speed Pulse Shape Processing
利用高速脉冲整形处理降低宇宙X射线探测器的本底
批准号:
03640249
负责人:
HAYASHIDA Kiyoshi
金额:
$0.13万
依托单位:
依托单位国家:
日本
项目类别:
Grant-in-Aid for General Scientific Research (C)
财政年份:
1991
资助国家:
日本
项目状态:
已结题
起止时间:
1991 至 1992

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中文摘要
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英文摘要
We have studied digital processing techniques for the pulse shapes of the output signals from X-ray counters. Our first motivation was to reduce particle backgrounds in the proportional counter more efficiently than with usual rise time discrimination method. However, in the course of the study, we noticed that polarimetry of X-ray photons can be done by means of the pulse shape processing (analysis). The basic idea was due to the fact that photoelectrons are preferentially emitted to the direction parallel to the electric vector of the incoming photons. If energy of photoelectron is high enough to reflect its direction of emission to the elongation of the primary electron cloud, pulse shape would be different depending on the geometry between the emission direction and the anode wire. It is expected that for X-ray photons with electric vector parallel to the anode wire the output pulse rises more rapidly than for the vertical case, on average.To examine the idea of "pulse shape (or ri … More se time) X-ray polarimetor", we performed experiments at the synchrotron facility in the Institute for High Energy Physics, Tsukuba, Japan. We irradiated a Xe filled proportional counter against the monochromatic X-ray beam there. Output signals from the preamplifier of the counter were sampled using a Digital Storage Scope. The pulse shape data stored in a personal computer system were analyzed. Rise time of the pulse was investigated, and for X- ray energy from 20 keV to 40 keV, it was found that the average rise time (10%-50% of the pulse peak) was shorter for the parallel (electric vector // anode wire) case. One problem was that reproducibility of the absolute values of the rise time was not good.There are handful of techniques for X-ray poralimetry. To get higher sensitivity for polarization, scattering methods (e. g. Bragg crystal) would be better. However, as for X-ray astronomy use, polarimetry with proportional counter and pulse shape analysis have advantages of 1) photons in wide energy bands can be measured, 2) spectral & timing information is obtained at the same time. Thus further study will enable this technique for actual use. Less
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H.TSUNEMI et al.: "Detction of X-ray polarization with a charge coupled device" Nucler Instruments and Methods in Physics Research. A321. 629-631 (1992)
H.TSUNEMI 等人:“用电荷耦合器件检测 X 射线偏振”核子仪器和物理研究方法。
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H. Tsunemi et al: "Detection of X-ray polarization with a charge coupled device" Numclear Instruments and Methods in Physics Research. A321. 629-631 (1992)
H. Tsunemi 等人:“用电荷耦合器件检测 X 射线偏振”Numclear 物理研究仪器和方法。
DOI: --
发表时间:
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通讯作者:
Development of Wideband X-ray Imaging Polarimeters and Hard X-ray Polarimetry
  • 批准号:
    23340071
  • 项目类别:
    Grant-in-Aid for Scientific Research (B)
  • 资助金额:
    $12.65万
  • 财政年份:
    2011
  • 负责人:
    HAYASHIDA Kiyoshi
  • 依托单位:
Measurement of size of super massive black holes through observation of X-ray variabilities
  • 批准号:
    14340061
  • 项目类别:
    Grant-in-Aid for Scientific Research (B)
  • 资助金额:
    $6.14万
  • 财政年份:
    2002
  • 负责人:
    HAYASHIDA Kiyoshi
  • 依托单位:
海外基金