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New techniques for imaging photon-counting and particle detectors.

机译:成像光子计数和粒子检测器的新技术。

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摘要

Since the advent of space-based astronomy in the early 1960's, there has been a need for space-qualified detectors with sufficient sensitivity and resolution to detect and image single photons, ions or electrons. This thesis describes a research programme to develop detectors that fulfil these requirements. I begin by describing the role of detectors in space astronomy and follow with a review of detector technologies, with particular emphasis on imaging techniques. Conductive charge division image readouts offer high performance, simplicity, and flexibility and their potential is investigated in both theory and practice. I introduce the basic design concept and discuss the fundamental factors limiting performance in relation to physical design and to underlying physical processes. Readout manufacturing techniques are reviewed and a novel method presented. I describe specific space and ground-based readout applications which proved valuable in teaching lessons and raising questions. These questions initiated an experimental programme, whose goals were to understand limiting physical processes and find techniques to overcome them. Results are presented, and the innovation of the progressive geometry readout technique, which this programme also spawned, is described. Progressive geometry readout devices, such as the Vernier anode, offer dramatically improved performance and have been successfully flight-proven. I describe the development of a Vernier readout for the J-PEX sounding rocket experiment, and discuss the instrument calibration and the flight programme. First investigations into a next generation of charge division readout design are presented. These devices will use charge comparison instead of amplitude measurement to further enhance resolution and count rate capability. In conclusion, I summarize the advances made during the course of this research, and discuss ongoing technological developments and further work which will enable MCP detectors to continue to excel where characteristics such as true photon-counting ability, high spatial resolution, format flexibility, and high temporal resolution are required.
机译:自从1960年代初基于天文的天文学问世以来,就需要一种具有空间灵敏度的,具有足够灵敏度和分辨率的检测器,以检测和成像单个光子,离子或电子。本文描述了一个研究计划,以开发满足这些要求的探测器。我首先描述探测器在空间天文学中的作用,然后回顾探测器技术,尤其着重于成像技术。导电电荷划分图像读数提供高性能,简单性和灵活性,并且在理论和实践中都研究了它们的潜力。我将介绍基本设计概念,并讨论限制与物理设计和基础物理过程相关的性能的基本因素。回顾了读出的制造技术并提出了一种新颖的方法。我描述了特定的基于空间和地面的读取应用程序,这些应用程序在教课和提出问题方面被证明是有价值的。这些问题启动了一个实验计划,其目的是了解限制物理过程并找到克服它们的技术。给出了结果,并描述了该程序也产生的渐进式几何读出技术的创新。诸如Vernier阳极之类的渐进式几何读出设备可显着提高性能,并已成功地进行了飞行验证。我描述了用于J-PEX探空火箭实验的游标读出器的开发,并讨论了仪器校准和飞行程序。提出了对下一代电荷分配读出设计的初步研究。这些设备将使用电荷比较而不是幅度测量来进一步提高分辨率和计数率功能。总之,我总结了研究过程中取得的进展,并讨论了正在进行的技术发展和进一步的工作,这些工作将使MCP检测器在真正的光子计数能力,高空间分辨率,格式灵活性和需要高时间分辨率。

著录项

  • 作者单位

    University of London, University College London (United Kingdom).;

  • 授予单位 University of London, University College London (United Kingdom).;
  • 学科 Astronomy.
  • 学位 Ph.D.
  • 年度 2004
  • 页码 304 p.
  • 总页数 304
  • 原文格式 PDF
  • 正文语种 eng
  • 中图分类
  • 关键词

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