LISA Telescope Assembly Optical Stability Characterization for ESA

被引:8
作者
Verlaan, Adrianus L. [1 ]
Hogenhuis, Harmen [1 ]
Pijnenburg, Joep [1 ]
Lemmen, Martin [1 ]
Lucarelli, Stefano [2 ]
Scheulen, Dietmar [2 ]
Ende, David [3 ]
机构
[1] TNO, Stieltjesweg 1,Postbus 155, NL-2600 AD Delft, Netherlands
[2] EADS ASTRIUM, D-88039 Friedrichshafen, Germany
[3] Xper Aerosp GmbH, D-88090 Immenstaad, Germany
来源
MODERN TECHNOLOGIES IN SPACE-AND GROUND-BASED TELESCOPES AND INSTRUMENTATION II | 2012年 / 8450卷
关键词
LISA; NGO; telescope; characterization;
D O I
10.1117/12.925112
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
The LISA Optical Stability Characterization project is part of the LISA CTP activities to achieve the required Technonlogy Readiness Level (TRL) for all of the LISA technologies used. This activity aims demonstration of the Telescope Assembly (TA), with a structure based on CFRP technology, that a CTE of 10(-7) 1/K can be achieved with measures to tune the CTE to this level. In addition the demonstration is required to prove that the structure exhibits highly predictable mechanical distortion characteristics when cooling down to -90 degrees C, during outgassing in space and when going from 1g environment to 0g. This paper describes the test facilities as well as the first test results. A dedicated test setup is designed and realized to allow monitoring dimensional variations of the TA using three interferometers, while varying the temperature in a thermal vacuum chamber. Critical parameters of the verification setup are the length metrology accuracy in thermal vacuum and the thermal vacuum flexibility and stability. The test programme includes Telescope Assembly CTE measurements and thermal gradient characterization.
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页数:7
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