Overview of the LSST Active Optics System

被引：18

作者：

Neill, Douglas ^{[1
]}

Angeli, George ^{[1
]}

Claver, Chuck ^{[1
]}

Hileman, Ed ^{[1
]}

DeVries, Joseph ^{[1
]}

Sebag, Jacques ^{[1
]}

Xin, Bo ^{[1
]}

机构：

[1] Natl Opt Astron Observ, Tucson, AZ 85719 USA

来源：

MODELING, SYSTEMS ENGINEERING, AND PROJECT MANAGEMENT FOR ASTRONOMY VI | 2014年 / 9150卷

关键词：

LSST; active optics system; AOS;

D O I：

10.1117/12.2056553

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

The LSST will utilize an Active Optics System to optimize the image quality by controlling the surface figures of the mirrors (M1M3 and M2) and maintain the relative position of the three optical systems (M1M3 mirror, M2 mirror and the camera). The mirror surfaces are adjusted by means of figure control actuators that support the mirrors. The relative rigid body positions of M1M3, M2 and the camera are controlled through hexapods that support the M2 mirror cell assembly and the camera. The Active Optics System (AOS) is principally operated off of a Look-Up Table (LUT) with corrections provided by wave front sensors.

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页数：16

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