Debris collision mitigation from the ground using laser guide star adaptive optics at mount Stromlo observatory

被引:2
|
作者
Martinez, N. [1 ,2 ]
D'Orgeville, C. [1 ,2 ]
Grosse, D. [1 ,2 ]
Lingham, M. [1 ,2 ]
Webb, J. [1 ,2 ]
Copeland, M. [1 ,2 ]
Galla, A. [1 ]
Hart, J. [1 ]
Price, I [1 ]
Schofield, W. [1 ]
Thorn, E. [3 ]
Smith, C. [2 ,3 ]
Gao, Y. [2 ,3 ]
Wang, Y. [2 ,3 ]
Blundell, M. [3 ]
Chan, A. [3 ]
Gray, A. [3 ]
Fetzer, G. [4 ]
Rako, S. [4 ]
机构
[1] Australian Natl Univ, Res Sch Astron & Astrophys, Mt Stromlo Observ, Cotter Rd, Weston 2611, Australia
[2] Space Environm Res Ctr, Mt Stromlo Observ, Cotter Rd, Weston 2611, Australia
[3] EOS Space Syst Pty Ltd, Symonston, Australia
[4] Arete, 2500 Trade Ctr Ave,Suite A, Longmont, CO 80503 USA
来源
JOURNAL OF SPACE SAFETY ENGINEERING | 2022年 / 9卷 / 01期
关键词
Debris collision mitigation; Adaptive optics; Laser guide star;
D O I
10.1016/j.jsse.2021.10.007
中图分类号
V [航空、航天];
学科分类号
08 ; 0825 ;
摘要
The Australian National University (ANU) and industry partners EOS Space Systems and Lockheed Martin are part of the Space Environment Research Centre (SERC), an Australian-Government funded cooperative research centre headquartered in Canberra, Australia. SERC aims to mitigate the threat of collisions with space debris using a ground-based high power (10-20kW) infrared (IR) laser to modify the debris orbit should a collision be predicted. To that end, the ANU has equipped the EOS 1.8m laser tracking station telescope on the ANU Mount Stromlo campus with a state-of-the-art Laser Guide Star Adaptive Optics (LGS AO) system to pre-compensate the IR laser prior to propagation through earth's atmosphere. The ANU LGS AO system is currently being integrated with the EOS telescope and the high-power IR laser. This paper provides a brief overview of the LGS AO system and focus more specifically on the design, integration and commissioning of the first LGS facility ever constructed in Australia. The LGS Facility includes two sodium guide star laser sources which can be either propagated separately or combined so as to produce a brighter reference star to maximise adaptive optics correction. The two lasers, their beam combining optics, their common beam transfer optics, and the laser launch telescope are hereby described.
引用
收藏
页码:106 / 113
页数:8
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