在PANTER对雅典娜光学系统进行x射线测试

V. Burwitz, G. Vacanti, M. Collon, N. Barrière, M. Bavdaz, I. Ferreira, M. Ayre, Emily Tipper, J. Eder, E. Breunig, G. Hartner, A. Langmeier, T. Müller, S. Rukdee, T. Schmidt
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引用次数: 4

摘要

硅孔光学(SPO)镜像模块(mm)正在为欧空局的雅典娜任务开发和生产。这些光学器件已经并将在MPEs PANTER x射线测试设备上进行测试。我们介绍了在PANTER x射线测试设备上对SPO MM-0050进行的测试结果,该测试是为了验证SPO的最新光学性能(半能宽(HEW),有效面积),支持欧空局对其光学性能的审查。PANTER、ESA、cosine和Media Lario的准备工作正在进行中,以对最终ATHENA镜组件结构的两个全尺寸1/6部分进行复杂的光热机械测试,该结构由潜在的ATHENA主要供应商空中客车防务和空间公司和泰利斯阿莱尼亚空间公司生产。为了这些测试,按照飞行配置生产了一套三枚SPO mm。mm将被整合到全尺寸的1/6扇区中,以测量热梯度对结构热弹性变形的影响,从而测量HEW性能。这里给出了测试的描述。PANTER还参与了镜适配器结构(MAS)的开发、测试和制造,以在XRCF计划的x射线测试期间支持2.6米直径的ATHENA镜组装模块演示(MAMD)。本文将介绍PANTER测试和结果的描述,以及XRCF的MAS MGSE的简要概述。
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X-ray testing ATHENA optics at PANTER
Silicon pore optic (SPO) mirror modules (MMs) are being developed and produced for ESA’s ATHENA mission. The optics have, and will be, tested at MPEs PANTER x-ray test facility. We present the results obtained from tests performed at the PANTER x-ray test facility for the SPO MM-0050 that was produced to verify the latest optical performance (half energy width (HEW), effective area) of SPOs, supporting the ESA reviews of their optical performance. The preparations are ongoing at PANTER, ESA, cosine and Media Lario to perform complex opto-thermo-mechanical tests of the two full scale 1/6th sectors of the final ATHENA mirror assembly structure produced by the potential ATHENA primes Airbus Defence and Space and Thales Alenia Space. For these tests a set of three SPO MMs have been produced following the flight configuration. The MMs will be incorporated into the full scale 1/6th sectors to measure the impact of thermal gradients on the thermoelastic deformation of the structure and therefore the HEW performance. A description of the tests is presented here. PANTER is also involved in the development, testing, and fabrication of the mirror adapter structure (MAS) to support the 2.6-m diameter ATHENA mirror assembly module demonstrators (MAMD) during the planned x-ray tests at XRCF. A description of the PANTER tests and results will be presented in this paper together with a short overview of the MAS MGSE for XRCF.
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