Picometer Level Spatial Metrology for Next Generation Telescopes

被引:2
|
作者
Saif, Babak [1 ]
Keski-Kuha, Ritva [1 ]
Greenfield, Perry [2 ]
North-Morris, Michael [3 ]
Bluth, Marcel [4 ]
Feinberg, Lee [1 ]
Wyant, J. C. [5 ]
Park, S. [6 ]
机构
[1] NASA, Goddard Space Flight Ctr, Greenbelt, MD 20771 USA
[2] Space Telescope Sci Inst, 3700 San Martin Dr, Baltimore, MD 21218 USA
[3] 4D Technol, 3280 E Hemisphere Loop,Suite 146, Tucson, AZ 85706 USA
[4] Intuit Machines, 3700 Bay Area Blvd,Suite 100, Houston, TX 77058 USA
[5] Univ Arizona, James C Wyant Coll Opt Sci, 1630 E Univ Blvd, Tucson, AZ 85721 USA
[6] Smithsonian Astrophys Observ, Cambridge, MA 02138 USA
关键词
JWST; interferometer; optical testing;
D O I
10.1117/12.2543034
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
Future space observatory missions require controlling wave front error and system alignment stability to picometer scale. Picometer stability performance demands precision knowledge of the mirror and metering structure materials to the same level. A high-speed electronic speckle pattern interferometer was designed and built to demonstrate measurements of both static and dynamic responses of picometer level amplitudes in mirror and structural materials subjected to very low energy disturbances. This paper summarizes the current status of tests to impart a dynamic disturbance of picometer scale and measure the response of specular and diffuse materials. The results show that subpicometer scale effects can be accurately measured in an open test environment outside a vacuum chamber.
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页数:8
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