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

基本信息

  • 批准号:
    03640249
  • 负责人:
  • 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
  • 起止时间:
    1991 至 1992
  • 项目状态:
    已结题

项目摘要

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
我们研究了 X 射线计数器输出信号脉冲形状的数字处理技术。我们的第一个动机是比通常的上升时间辨别方法更有效地减少正比计数器中的粒子背景。然而,在研究过程中,我们注意到X射线光子的偏振测量可以通过脉冲形状处理(分析)来完成。基本思想是由于光电子优先发射到与入射光子的电矢量平行的方向。如果光电子的能量足够高以将其发射方向反映到初级电子云的伸长,则脉冲形状将根据发射方向和阳极线之间的几何形状而不同。平均而言,对于电矢量平行于阳极线的 X 射线光子,输出脉冲的上升速度比垂直情况更快。为了检验“脉冲形状(或 ri … More se 时间)X 射线偏振计”的想法,我们在日本筑波高能物理研究所的同步加速器设施中进行了实验。我们用 Xe 填充正比计数器照射单色 X 射线束。使用数字存储示波器对计数器前置放大器的输出信号进行采样。对存储在个人计算机系统中的脉冲形状数据进行了分析。研究了脉冲的上升时间,对于从 20 keV 到 40 keV 的 X 射线能量,发现并联(电矢量/阳极线)情况下的平均上升时间(脉冲峰值的 10%-50%)较短。一个问题是上升时间绝对值的再现性不好。X 射线偏振测定技术有几种。为了获得更高的偏振灵敏度,散射方法(例如布拉格晶体)会更好。然而,对于X射线天文学用途,采用正比计数器和脉冲形状分析的偏振测量具有以下优点:1)可以测量宽能带中的光子,2)同时获得光谱和定时信息。因此,进一步的研究将使该技术能够实际使用。较少的

项目成果

期刊论文数量(2)
专著数量(0)
科研奖励数量(0)
会议论文数量(0)
专利数量(0)
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。
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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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    0
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HAYASHIDA Kiyoshi其他文献

HAYASHIDA Kiyoshi的其他文献

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{{ truncateString('HAYASHIDA Kiyoshi', 18)}}的其他基金

Development of Wideband X-ray Imaging Polarimeters and Hard X-ray Polarimetry
宽带X射线成像旋光仪和硬X射线旋光仪的研制
  • 批准号:
    23340071
  • 财政年份:
    2011
  • 资助金额:
    $ 0.13万
  • 项目类别:
    Grant-in-Aid for Scientific Research (B)
Measurement of size of super massive black holes through observation of X-ray variabilities
通过观测X射线变异测量超大质量黑洞的尺寸
  • 批准号:
    14340061
  • 财政年份:
    2002
  • 资助金额:
    $ 0.13万
  • 项目类别:
    Grant-in-Aid for Scientific Research (B)

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Extremely efficient fully three-dimensional hydrodynamic simulations of supernova remnants for the new age of microcalorimetric X-ray astronomy
针对微量热 X 射线天文学新时代的超新星遗迹进行极其高效的全三维流体动力学模拟
  • 批准号:
    24K07092
  • 财政年份:
    2024
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    Grant-in-Aid for Scientific Research (C)
Optimizing telescope design for X-ray astronomy missions
优化 X 射线天文学任务的望远镜设计
  • 批准号:
    2438212
  • 财政年份:
    2020
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    Studentship
The application of deep learning to X ray astronomy
深度学习在X射线天文学中的应用
  • 批准号:
    2022929
  • 财政年份:
    2017
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    $ 0.13万
  • 项目类别:
    Studentship
Measurement of the ion stopping power of hydrogen atoms using a high resolution spectrometer for x-ray astronomy
使用 X 射线天文学高分辨率光谱仪测量氢原子的离子阻止本领
  • 批准号:
    16K17686
  • 财政年份:
    2016
  • 资助金额:
    $ 0.13万
  • 项目类别:
    Grant-in-Aid for Young Scientists (B)
IoA Theoretical and X-ray Astronomy consolidation
IoA 理论和 X 射线天文学巩固
  • 批准号:
    ST/J001538/1
  • 财政年份:
    2012
  • 资助金额:
    $ 0.13万
  • 项目类别:
    Research Grant
X-Ray Astronomy, Galaxy Clusters, Cosmology
X射线天文学、星系团、宇宙学
  • 批准号:
    158967163
  • 财政年份:
    2010
  • 资助金额:
    $ 0.13万
  • 项目类别:
    Heisenberg Professorships
X-Ray Astronomy, Galaxy Clusters, Cosmology
X射线天文学、星系团、宇宙学
  • 批准号:
    158967534
  • 财政年份:
    2010
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    $ 0.13万
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From X-ray astronomy to gamma scintigraphy: a high resolution gamma camera for medical imaging
从 X 射线天文学到伽马闪烁扫描:用于医学成像的高分辨率伽马相机
  • 批准号:
    G0802647/1
  • 财政年份:
    2009
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Study of solar X-ray albedo by the upper earth atmosphere and fluorescent X-rays using the data obtained by the X-ray astronomy satellite
利用X射线天文卫星获得的数据研究上层地球大气和荧光X射线的太阳X射线反照率
  • 批准号:
    12640433
  • 财政年份:
    2000
  • 资助金额:
    $ 0.13万
  • 项目类别:
    Grant-in-Aid for Scientific Research (C)
X-Ray Astronomy Study with the Astro-E Satellite
使用 Astro-E 卫星进行 X 射线天文学研究
  • 批准号:
    10044102
  • 财政年份:
    1998
  • 资助金额:
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