X-ray telescope design and technology: what the future holds

被引：0
|
作者：
Willingale, Richard [1 ]
机构：
[1] Univ Leicester, Dept Phys & Astron, Leicester LE1 7RH, Leics, England
来源：
SPACE TELESCOPES AND INSTRUMENTATION 2010: ULTRAVIOLET TO GAMMA RAY | 2010年 / 7732卷
关键词：
X-ray optics for astronomy; XMM-NEWTON; ASTRONOMY; OPTICS; PERFORMANCE; MIRRORS; LENSES; SYSTEM;
D O I：
10.1117/12.861348
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
The great X-ray Observatories of the 20th Century relied exclusively on the Wolter Type I optics design to provided true imaging in the energy band 0.1-10 keV. What are the prospects for continued development of the W-I geometry in the 21st Century and what alternative designs, technologies and bright ideas maybe poised to make an impact in X-ray astronomy in the future?
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页数：8
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