MMT望远镜6.5m转换自适应二次系统设计现状

Adaptive Optics Pub Date : 1900-01-01 DOI:10.1364/adop.1996.athc.17

G. Brusa, P. Gray, C. Vecchio, P. Salinari, W. Gallieni

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引用次数: 0

摘要

使用自适应次镜进行天文高分辨率观测的优点是非常吸引人的。沿着自适应系统的光学序列的光学表面的急剧减少将允许一个非常紧凑的系统具有高透射率和低发射率。此外，这样的系统具有非常高的致动器密度的潜力。

本文章由计算机程序翻译，如有差异，请以英文原文为准。

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Status of the Design of an Adaptive Secondary for the 6.5m conversion of the MMT telescope

The advantages of using an adaptive secondary mirror for astronomical high resolution observations are very attractive. The drastic reduction of optical surfaces along the optical train of the adaptive system will allow a very compact system with high transmission and low emissivity. Also such a system has the potentiality of a very high actuator density.

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Adaptive Optics

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