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Development of a cryogenic laboratory for the testing of the ISO optical subsystem

机译:用于测试ISO光学子系统的低温实验室的开发

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Since the beginning of 1988, the Focal 5 facility of CSL (Centre Spatial de Liege) has been upgraded in order to perform the cryogenic optical tests of the single optical components as well as the overall telescope assembly of the optical subsystem of the ESA ISO telescope. The main objectives of these vacuum thermal tests were: 1. to measure the optical surface quality of the various components and of the fully assembled telescope (WFE measurement at cryogenic temperatures (5k); and 2. to measure the misalignment of the telescope and its associated experiments when in cryogenic conditions (5k). Consequently, a special experimental set-up has been designed and manufactured in order to reach these objectives taking into account that: 1. Alignment between the different optical elements had to be kept during the cryo-test inside given ranges (+/- 15 arcmin) from 300k to 5k; 2. The cool down and the warm-up phases of the specimens had not to induce excessive constrains in the materials; 3. The measurements were achieved through interferometric methods which required high stability; and 4. Special care had to be taken for the thermal control, thermal monitoring and thermal measurements.
机译:自1988年开始,焦点5设施CSL的(中心空间解列日)已经升级,以便组件执行单个光学部件的低温光学测试以及整体望远镜的ESA ISO望远镜的光学子系统的。这些真空热测试的主要目标是:1.测量各种组件的光学表面质量和完全装配的望远镜(在低温下的测量WFE(5K);以及2.测量望远镜和的未对准其相关联的实验在低温条件时(5K)。因此,一个特殊的实验设置的设计和为了达到这些目标考虑到制造的:1.不同的光学元件之间的对准有cryo-期间被保持测试里面给定的范围(+/- 15弧分)从300K至5K; 2.冷却和试样的热身阶段没有诱导过度约束在材料; 3.该测量通过干涉的方法来实现,其所需的高稳定性;和4.特殊护理必须采取用于热控制,热监视及热测量。

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