Golden L J
Appl Opt. 1975 Oct 1;14(10):2391-9. doi: 10.1364/AO.14.002391.
The dynamic Hartmann test was developed to monitor precisely the alignment and optical figure of a complete telescope system such as the Large Space Telescope by using a real star source. The test was chosen for its large range of operation, sensitivity, and relative simplicity. The dynamic Hartmann test configuration is discussed and analyzed, and the construction of an experimental test instrument is described. A wavefront error simulator is used to determine experimentally the capability of the Hartmann test instrument in detecting low-order aberrations under laboratory conditions. It is found that sensitivities in the lambda/50 to lambda/100 range can be realized.
动态哈特曼测试的开发是为了通过使用真实恒星源精确监测诸如大型空间望远镜等完整望远镜系统的对准情况和光学外形。选择该测试是因其操作范围广、灵敏度高且相对简单。文中讨论并分析了动态哈特曼测试配置，还描述了一台实验测试仪器的构造。使用一个波前误差模拟器在实验室条件下通过实验确定哈特曼测试仪器检测低阶像差的能力。结果发现，可以实现λ/50至λ/100范围内的灵敏度。
