使用气凝胶切伦科夫探测器对天鹅座x射线产生的时间分辨测量

Y. Kim, H. Herrmann, M. Kaufman, R. Howe, C. Young, R. Malone, J. A. Green, T. Haines
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摘要

天鹅座气凝胶切伦科夫探测器(ACD/C)已经开发出来,可以提供天鹅座的时间相关x射线光谱信息,天鹅座是内华达州国家安全基地运行的强烈闪光x射线源。在三个能量阈值下测量时间分辨天鹅座x射线信号:1.3 MeV (197 mg/cc气凝胶),1.1 MeV (260 mg/cc气凝胶)和0.3 MeV(石英)。ACD/C数据定性地表明高能x射线峰存在于比天鹅座电压或电流脉冲更短的时间尺度上。随时间变化的x射线光谱信息可以提高对致密物体射线照相的物理理解。
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Time-resolved measurements of Cygnus x-ray production using Aerogel Cherenkov Detector
An Aerogel Cherenkov Detector for Cygnus (ACD/C) has been developed to provide time-dependent x-ray spectral information from Cygnus — an intense flash x-ray source operated at the Nevada National Security Site. Time-resolved Cygnus x-ray signals were measured at three energy thresholds: 1.3 MeV (by 197 mg/cc aerogel), 1.1 MeV (by 260 mg/cc aerogel), and 0.3 MeV (by quartz). ACD/C data qualitatively suggest that the high-energy x-ray peak exists on a shorter timescale than the Cygnus voltage or current pulse. A time-dependent, x-ray spectral information can improve the understanding of the physics of dense objects radiography.
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