Development status of adjustable grazing incidence optics for 0.5 arcsecond X-ray imaging

被引:17
作者
Reid, Paul B. [1 ]
Aldcroft, Thomas L. [1 ]
Allured, Ryan [1 ]
Cotroneo, Vincenzo [1 ]
Johnson-Wilke, Raegan L. [2 ]
Marquez, Vanessa [1 ]
McMuldroch, Stuart [1 ]
O'Dell, Stephen L. [3 ]
Ramsey, Brian D. [3 ]
Schwartz, Daniel A. [1 ]
Trolier-McKinstry, Susan [2 ]
Vikhlinin, Alexey [1 ]
Wilke, Rudeger H. T. [2 ]
Zhao, Rui [2 ]
机构
[1] Harvard Smithsonian Ctr Astrophys, 60 Garden St, Cambridge, MA 02138 USA
[2] Penn State Univ, University Pk, PA 16802 USA
[3] NASA Marshall Space Flight Ctr, Astrophys Off ZP12, Huntsville, AL 35812 USA
来源
ADAPTIVE X-RAY OPTICS III | 2014年 / 9208卷
关键词
x-ray optics; adjustable optics; active optics; piezoelectric; deformable mirrors; SMART-X; high resolution; lightweight optics;
D O I
10.1117/12.2063305
中图分类号
O43 [光学];
学科分类号
070207 ; 0803 ;
摘要
We describe progress in the development of adjustable grazing incidence X-ray optics for 0.5 arcsec resolution cosmic X-ray imaging. To date, no optics technology is available to blend high resolution imaging like the Chandra X-ray Observatory, with square meter collecting area. Our approach to achieve these goals simultaneously is to directly deposit thin film piezoelectric actuators on the back surface of thin, lightweight Wolter-I or Wolter-Schwarschild mirror segments. The actuators are used to correct mirror figure errors due to fabrication, mounting and alignment, using calibration and a one-time figure adjustment on the ground. If necessary, it will also be possible to correct for residual gravity release and thermal effects on-orbit. In this paper we discuss our most recent results measuring influence functions of the piezoelectric actuators using a Shack-Hartmann wavefront sensor. We describe accelerated and real-time lifetime testing of the piezoelectric material, and we also discuss changes to, and recent results of, our simulations of mirror correction.
引用
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页数:9
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