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Thermal, structural, and optical analysis of a balloon-based imaging system.

Borden, M. and Lewis, D. and Ochoa, H. and Jones-Wilson, L. and Susca, S. and Porter, M. and Massey, R. and Clark, P. and Netterfield, B. (2017) 'Thermal, structural, and optical analysis of a balloon-based imaging system.', Publications of the Astronomical Society of the Pacific., 129 . 035001.

Abstract

The Subarcsecond Telescope And BaLloon Experiment, STABLE, is the fine stage of a guidance system for a high-altitude ballooning platform designed to demonstrate subarcsecond pointing stability over one minute using relatively dim guide stars in the visible spectrum. The STABLE system uses an attitude rate sensor and the motion of the guide star on a detector to control a Fast Steering Mirror to stabilize the image. The characteristics of the thermal-optical-mechanical elements in the system directly affect the quality of the point-spread function of the guide star on the detector, so a series of thermal, structural, and optical models were built to simulate system performance and ultimately inform the final pointing stability predictions. This paper describes the modeling techniques employed in each of these subsystems. The results from those models are discussed in detail, highlighting the development of the worst-case cold and hot cases, the optical metrics generated from the finite element model, and the expected STABLE residual wavefront error and decenter. Finally, the paper concludes with the predicted sensitivities in the STABLE system, which show that thermal deadbanding, structural pre-loading, and self-deflection under different loading conditions, and the speed of individual optical elements were particularly important to the resulting STABLE optical performance.

Item Type:Article
Full text:(AM) Accepted Manuscript
First Live Deposit - 17 March 2017
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Status:Peer-reviewed
Publisher Web site:https://doi.org/10.1088/1538-3873/129/973/035001
Publisher statement:This is an author-created, un-copyedited version of an article published in Publications of the Astronomical Society of the Pacific. IOP Publishing Ltd is not responsible for any errors or omissions in this version of the manuscript or any version derived from it. The Version of Record is available online at https://doi.org/10.1088/1538-3873/129/973/035001
Record Created:17 Mar 2017 15:43
Last Modified:21 Jan 2018 00:54

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