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  点击该按纽隐藏左边的页面菜单以便扩大工作区域的面积

干涉仪与波前探测系统比较
 Optino 波前测试系统相对于干涉仪的优点
  干涉仪 Optino 波前系统
1购买、运行、维护费用高非常便宜
2系统体积大,需要大型光学平台结构紧凑,普通桌子就可以
3需要昂贵的隔振平台非常耐用,无需隔振,普通桌子就可以,即使重击桌子也不会影响测试结果或仪器性能
4需要洁净室普通干净的实验室环境足够了
5需要控制测试现场的气流可以在紧靠打磨机器工作现场使用
6需要激光光源普通光源或激光均可
7由于激光波长范围有限,只能工作在有限的几个波长任何波长均可工作,从193nm到1700nm,软件功能不受波长和配置的影响
8仅限于测试平面、球面及浅度非球面测试可以测试深度非球面元件(球形失常值达50λ
9不能测试非规则形状元件可以测试非规则元件,如柱面镜
10动态范围受CCD探测器上干涉条纹限制,方法本身具有高动态特性
 Optino Pro vs. Zygo GPI xp HR Interferometer:

通过使用Zygo GPI xp HR干涉仪和Spot-Optics公司的Optino 波前测试系统对一个硬盘上小面积(7mm)区域,进行测试对比。

右图白色圆圈位置的区域即为测试区域,是一个平整的表面,测试的波长为632nm,下图为主要测试得到的参数对比:

 
 
 
  
 去除了倾斜(Tilt), Piston and 散焦 (defocus)影响后的表面3D形貌图( Zygo )
 去除了倾斜和散焦的3D表面形貌图(Optino)
由上可见:基于Shack-Hartmann 测试原理的Optino 可以获得与Zygo干涉仪一致的测试结果
应用说明
卡式 Cassegrain 焦点测试
 
 测试配置说明:
A telescope tested at the Cassegrain focus using external parallel light. The aberrations of the SH system itself are removed by taking a calibration frame, with a calibration source placed at the focus of Puntino. The incident light illuminating the system should be aberration free. In the case of an astronomical telescope, a natural star is used.

It is not necessary to use parallel light for the test. The measured aberrations will then no longer refer to those for parallel light, but to one particular optical configuration that is used for the test.
 
 
 牛顿焦点 Newtonian focus 测试
 
测试配置说明
A telescope tested at the Newtonian focus using parallel light. The aberrations of the SH system itself are removed by taking a calibration frame, with a calibration source placed at the focus of Puntino. The incident light illuminating the system should be aberration free. In the case of an astronomical telescope, a natural star is used.

It is not necessary to use parallel light for the test. The measured aberrations will then no longer refer to those for parallel light, but to one particular optical configuration that is used for the test.
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