首页> 外文会议>Conference on Ground-Based Telescopes pt.2; 20040621-20040625; Glasgow; GB >Active Optics and Wavefront Sensing at the Upgraded 6.5-meter MMT
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Active Optics and Wavefront Sensing at the Upgraded 6.5-meter MMT

机译:升级后的6.5米MMT上的有源光学和波前传感

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摘要

Shack-Hartmann wavefront sensors have been commissioned and are now in routine use at both of the optical foci (f/9 and f/5) of the converted MMT. Both units are of moderate resolution with 14x14 square apertures across the pupil for f/5 and 13x13 hexagonal apertures for f/9. They share a common software interface that fits a set of 19 Zernike polynomials to the wavefront errors. Zernike focus and coma are corrected by moving the secondary mirror, third order spherical by a combination of secondary motion and primary bending, and the rest by primary bending alone. In this paper we will describe the two wavefront sensor systems and how they have performed thus far.
机译:Shack-Hartmann波前传感器已经调试,现在已在转换后的MMT的两个光学焦点(f / 9和f / 5)上常规使用。两种单位的分辨率均中等,f / 5时瞳孔上的14x14方形孔径,f / 9时的13x13六角形孔径。它们共享一个通用的软件界面,该界面适合一组19个Zernike多项式以适应波前误差。 Zernike的焦点和昏迷可通过移动辅助镜,通过辅助运动和一次弯曲的组合来移动三阶球面以及通过单独进行一次弯曲来移动其余部分来校正。在本文中,我们将描述两个波前传感器系统及其迄今为止的性能。

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