Activation in the COMPTEL double-scattering gamma-ray telescope

D. Morris, M. McConnell, J. Ryan, R. Diehl, U. Oberlack, V. Schonfelder, M. Varendorff, G. Weidenspointner, H. de Boer, K. Bennett
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引用次数: 0

Abstract

The COMPTEL gamma-ray telescope has been operating in low Earth orbit for six years, since the launch of the Compton Gamma-Ray Observatory in April 1991. Comparisons of data for different orbits and epochs show evidence of activation on time scales from minutes (/sup 27/Mg, /spl tau//sub 1/2/=9.5 min) to years (/sup 22/Na, /spl tau//sub 1/2/=2.58 yr). The activation is correlated with both the orbital altitude and solar cosmic-ray modulation. Because it requires coincident measurements in two different detectors, COMPTEL is most susceptible to instrumental background events in which two or more photons are produced simultaneously.
COMPTEL双散射伽玛射线望远镜的激活
康普顿伽玛射线天文台于1991年4月发射以来,康普顿伽玛射线望远镜已经在近地轨道运行了六年。对不同轨道和不同时期的数据进行比较,显示了在时间尺度上的激活证据,从分钟(/sup 27/Mg, /spl tau//sub 1/2/=9.5 min)到年(/sup 22/Na, /spl tau//sub 1/2/=2.58 yr)。激活与轨道高度和太阳宇宙射线调制有关。因为它需要在两个不同的探测器上进行同步测量,COMPTEL最容易受到同时产生两个或更多光子的仪器背景事件的影响。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
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