Ralf K. Heilmann, David P. Huenemoerder, Jake A. McCoy, Randall L. McEntaffer
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引用次数: 0
Abstract
X-ray diffraction gratings play an essential role in high-resolution
spectroscopy of astrophysical phenomena. We present some scientific highlights
from the X-ray grating spectrometers (XGS) on board of the Chandra and
XMM/Newton missions, XGS optical design, and the basic physics of grating
diffraction geometry and efficiency. We review design, fabrication, and
performance of the currently orbiting transmission and reflection grating
elements, followed by descriptions of the state-of-the art of more advanced
grating technologies that promise orders-of-magnitude improvements in XGS
performance, especially in combination with advanced X-ray telescope mirrors. A
few key science questions that require new grating technology are posed, and
powerful future mission concepts and recent and approved missions are
presented.
X射线衍射光栅在天体物理现象的高分辨率光谱分析中发挥着至关重要的作用。我们将介绍钱德拉和XMM/牛顿飞行任务所搭载的X射线光栅分光计(XGS)的一些科学亮点、XGS光学设计以及光栅衍射几何和效率的基本物理学原理。我们回顾了目前轨道上的透射和反射光栅元件的设计、制造和性能,随后介绍了更先进的光栅技术的最新进展,这些技术有望使 XGS 的性能提高几个数量级,特别是与先进的 X 射线望远镜反射镜结合使用时。提出了一些需要新光栅技术的关键科学问题,并介绍了强有力的未来飞行任务概念以及最近批准的飞行任务。