天体物理用硬x射线偏振计的研制

M. McConnell, J. Macri, M. McClish, J. Ryan, D. Forrest, W. Vestrand
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引用次数: 13

摘要

我们一直在开发一种康普顿散射偏振计,用于测量来自天体物理源的硬x射线(100-300 keV)的线性偏振。一个实验室原型偏振计已经成功地证明了我们的蒙特卡罗模拟代码的可靠性,并证明了我们在实验室中产生偏振光子源的能力。我们的设计理念是在5英寸位置敏感PMT (PSPMT)的前端放置一个独立的偏振计模块。我们目前正在制作一个基于PSPMT概念的科学模型。虽然我们的开发重点是测量来自太阳耀斑的硬x射线,但我们的设计有一个优势,即它比相当大的视场(>1个立体度)更敏感,这一特点使它对/spl伽马/射线爆发研究特别有吸引力。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
Development of a hard X-ray polarimeter for astrophysics
We have been developing a Compton scatter polarimeter for measuring the linear polarization of hard X-rays (100-300 keV) from astrophysical sources. A laboratory prototype polarimeter has been used to successfully demonstrate the reliability of our Monte Carlo simulation code and to demonstrate our ability to generate a polarized photon source in the lab. Our design concept places a self-contained polarimeter module on the front-end of a a 5-inch position sensitive PMT (PSPMT). We are currently working on the fabrication of a science model based on this PSPMT concept. Although the emphasis of our development effort is towards measuring hard X-rays from solar flares, our design has the advantage that it is sensitive over a rather large field-of-view (>1 steradian), a feature that makes it especially attractive for /spl gamma/-ray burst studies.
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