Design and qualification of an aluminum deformable mirror for spaceborne electro-optical payloads

IF 1.7 3区 工程技术 Q2 ENGINEERING, AEROSPACE
Yesh Pal, Naveen Kumar Mishra, Naimesh R. Patel, Neeraj Mathur, Shaunak R. Joshi
{"title":"Design and qualification of an aluminum deformable mirror for spaceborne electro-optical payloads","authors":"Yesh Pal, Naveen Kumar Mishra, Naimesh R. Patel, Neeraj Mathur, Shaunak R. Joshi","doi":"10.1117/1.jatis.10.3.039002","DOIUrl":null,"url":null,"abstract":"The goal of deformable mirrors (DMs) is to correct aberrated optical wavefronts in spaceborne electro-optical (EO) payloads. It is used as part of an active/adaptive optics system. A continuous-surface, metal-based DM is highly reliable and less complex to assemble, has better stability of the active surface, is less expensive, and can be manufactured quickly. In addition, metal DM with actuation away from the active surface makes the overall configuration scalable. Continuing our previous work on deformable metal mirrors, this work presents the design, validation, and qualification of an aluminum DM using 25 piezoelectric actuators, which include an actuator in the center of the mirror, to improve the spherical aberration correction accuracy. The optomechanical design and analysis of the deformable mirror assembly (DMA) are also presented for performance and survival loads. Later, a qualification model (QM) was built with vacuum-compatible closed-loop piezoelectric actuators. The correction accuracy was demonstrated at the QM by correcting aberrations in the mirror itself. The QM was successfully tested in the space environment in the ThermoVac for operating temperature limits of 20°C±5°C and demonstrated survivability for storage temperature limits of 20°C±40°C. Likewise, the survivability of QM for launch environments such as sinusoidal and random vibration loads is demonstrated. The successful completion of all these tests has improved the maturity of this technology to the technology readiness level of 7 and is now ready to be configured for the appropriate spaceborne EO payload.","PeriodicalId":54342,"journal":{"name":"Journal of Astronomical Telescopes Instruments and Systems","volume":null,"pages":null},"PeriodicalIF":1.7000,"publicationDate":"2024-07-01","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"0","resultStr":null,"platform":"Semanticscholar","paperid":null,"PeriodicalName":"Journal of Astronomical Telescopes Instruments and Systems","FirstCategoryId":"5","ListUrlMain":"https://doi.org/10.1117/1.jatis.10.3.039002","RegionNum":3,"RegionCategory":"工程技术","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"Q2","JCRName":"ENGINEERING, AEROSPACE","Score":null,"Total":0}
引用次数: 0

Abstract

The goal of deformable mirrors (DMs) is to correct aberrated optical wavefronts in spaceborne electro-optical (EO) payloads. It is used as part of an active/adaptive optics system. A continuous-surface, metal-based DM is highly reliable and less complex to assemble, has better stability of the active surface, is less expensive, and can be manufactured quickly. In addition, metal DM with actuation away from the active surface makes the overall configuration scalable. Continuing our previous work on deformable metal mirrors, this work presents the design, validation, and qualification of an aluminum DM using 25 piezoelectric actuators, which include an actuator in the center of the mirror, to improve the spherical aberration correction accuracy. The optomechanical design and analysis of the deformable mirror assembly (DMA) are also presented for performance and survival loads. Later, a qualification model (QM) was built with vacuum-compatible closed-loop piezoelectric actuators. The correction accuracy was demonstrated at the QM by correcting aberrations in the mirror itself. The QM was successfully tested in the space environment in the ThermoVac for operating temperature limits of 20°C±5°C and demonstrated survivability for storage temperature limits of 20°C±40°C. Likewise, the survivability of QM for launch environments such as sinusoidal and random vibration loads is demonstrated. The successful completion of all these tests has improved the maturity of this technology to the technology readiness level of 7 and is now ready to be configured for the appropriate spaceborne EO payload.
设计和鉴定用于空间电子光学有效载荷的铝质可变形反射镜
可变形反射镜(DM)的目标是校正空间电子光学(EO)有效载荷中的畸变光波面。它是主动/自适应光学系统的一部分。基于金属的连续表面 DM 可靠性高,组装不复杂,有源表面的稳定性更好,成本较低,可以快速制造。此外,远离有源表面的金属 DM 使整体配置具有可扩展性。本研究延续了我们之前在可变形金属镜方面的工作,介绍了使用 25 个压电致动器的铝制 DM 的设计、验证和鉴定,其中包括位于镜面中心的致动器,以提高球差校正精度。此外,还介绍了可变形反射镜组件(DMA)的光学机械设计和性能及生存负载分析。随后,利用真空兼容闭环压电致动器建立了一个合格模型(QM)。通过校正反射镜本身的像差,证明了 QM 的校正精度。QM 在空间环境中的 ThermoVac 成功进行了测试,工作温度限制为 20°C±5°C,并证明了其在 20°C±40°C存储温度限制下的生存能力。同样,还证明了 QM 在正弦和随机振动负载等发射环境中的生存能力。所有这些测试的成功完成将该技术的成熟度提高到了 7 级技术就绪水平,现在可以为适当的星载 EO 有效载荷进行配置。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
求助全文
约1分钟内获得全文 求助全文
来源期刊
CiteScore
4.40
自引率
13.00%
发文量
119
期刊介绍: The Journal of Astronomical Telescopes, Instruments, and Systems publishes peer-reviewed papers reporting on original research in the development, testing, and application of telescopes, instrumentation, techniques, and systems for ground- and space-based astronomy.
×
引用
GB/T 7714-2015
复制
MLA
复制
APA
复制
导出至
BibTeX EndNote RefMan NoteFirst NoteExpress
×
提示
您的信息不完整,为了账户安全,请先补充。
现在去补充
×
提示
您因"违规操作"
具体请查看互助需知
我知道了
×
提示
确定
请完成安全验证×
copy
已复制链接
快去分享给好友吧!
我知道了
右上角分享
点击右上角分享
0
联系我们:info@booksci.cn Book学术提供免费学术资源搜索服务,方便国内外学者检索中英文文献。致力于提供最便捷和优质的服务体验。 Copyright © 2023 布克学术 All rights reserved.
京ICP备2023020795号-1
ghs 京公网安备 11010802042870号
Book学术文献互助
Book学术文献互助群
群 号:481959085
Book学术官方微信