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arXiv 1807.01657astro-ph.IM
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LINC-NIRVANA地面和高层WFS的校准程序

The calibration procedure of the LINC-NIRVANA ground and high layer WFS

Carmelo Arcidiacono, Kalyan Kumar Radhakrishnan Santhakumari, Valentina Viotto, Maria Bergomi, Florian Briegel, Thomas Bertram, Luca Marafatto, Tom Herbst, Jaco… 展开作者

Carmelo Arcidiacono, Kalyan Kumar Radhakrishnan Santhakumari, Valentina Viotto, Maria Bergomi, Florian Briegel, Thomas Bertram, Luca Marafatto, Tom Herbst, Jacopo Farinato, Roberto Ragazzoni, Ralph Hofferbert, Martin Kuerster, Frank Kittman, Juergen Berwein, Harald Baumeister

摘要:

LINC--NIRVANA(LN)是一个MCAO模块,目前安装在大双目望远镜(LBT)的后弯格里高利焦点上。它安装了一个最初设计用于实现望远镜干涉成像焦点站的相机。LN遵循LBT双目策略,具有两个双通道:辅助双臂的双层定向多共轭自适应光学系统,提供高阶波前校正。为了平衡场旋转,对两个地波-波前传感器应用机械去旋,并且对两个高层传感器应用光学(K-镜)去旋,固定焦平面相对于波前传感器上的金字塔的位置。去旋转引入波前传感器上的光瞳图像旋转,从而改变可变形反射镜在传感器上的投影。

英文摘要:

LINC--NIRVANA (LN) is an MCAO module currently mounted on the Rear Bent Gregorian focus of the Large Binocular Telescope (LBT). It mounts a camera originally designed to realize the interferometric imaging focal station of the telescopes. LN follows the LBT binocular strategy having two twin channels: a double Layer Oriented Multi-Conjugate Adaptive Optics system assisting the two arms, supplies high order wave-front correction. In order to counterbalance the field rotation, a mechanical derotation is applied for the two ground wave-front sensors, and an optical (K-mirror) one for the two high layers sensors, fixing the positions of the focal planes with respect to the pyramids aboard the wavefront sensors. The derotation introduces a pupil images rotation on the wavefront sensors, changing the projection of the deformable mirrors on the sensor consequently.

机构、总结、中文摘要均由AI分析而来,可能存在错误,请以论文正文为准。

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