Aligning, Bonding, and Testing Mirrors for Lightweight X-ray Telescopes

被引:4
作者
Chan, Kai-Wing [1 ,2 ,4 ]
Zhang, William W. [4 ]
Saha, Timo T. [4 ]
McClelland, Ryan S. [3 ,4 ]
Biskach, Michael P. [3 ,4 ]
Niemeyer, Jason [3 ,4 ]
Schofield, Mark J. [3 ,4 ]
Mazzarella, James R. [3 ,4 ]
Kolos, Linette D. [4 ]
Hong, Melinda M. [3 ,4 ]
Numata, Ai [3 ,4 ]
Sharpe, Marton V. [3 ,4 ]
Solly, Peter M. [3 ,4 ]
Riveros, Raul E. [1 ,2 ,4 ]
Allgood, Kim D. [3 ,4 ]
McKeon, Kevin P. [3 ,4 ]
机构
[1] Ctr Res & Explorat Space Sci & Technol, Baltimore, MD 21250 USA
[2] Univ Maryland Baltimore Cty, Baltimore, MD 21250 USA
[3] Stinger Ghaffarian Technol Inc, Greenbelt, MD 20770 USA
[4] NASA, Goddard Space Flight Ctr, Greenbelt, MD 20771 USA
来源
OPTICS FOR EUV, X-RAY, AND GAMMA-RAY ASTRONOMY VII | 2015年 / 9603卷
关键词
X-ray optics; lightweight mirrors; segmented mirrors; mirror alignment; mirror bonding;
D O I
10.1117/12.2187016
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
High-resolution, high throughput optics for x-ray astronomy entails fabrication of well-formed mirror segments and their integration with arc-second precision. In this paper, we address issues of aligning and bonding thin glass mirrors with negligible additional distortion. Stability of the bonded mirrors and the curing of epoxy used in bonding them were tested extensively. We present results from tests of bonding mirrors onto experimental modules, and on the stability of the bonded mirrors tested in x-ray. These results demonstrate the fundamental validity of the methods used in integrating mirrors into telescope module, and reveal the areas for further investigation. The alignment and integration methods are applicable to the astronomical mission concept such as STAR-X, the Survey and Time-domain Astronomical Research Explorer.
引用
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页数:12
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