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Proceedings Paper

Ground-based stellar interferometry with adaptive optics
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Paper Abstract

A ground-based stellar interferometer appears to be a potentially useful research tool in studying stellar astrophysics and synthesizing a high resolution stellar image; however, its short-exposure performance is easily degraded by atmospheric turbulence. Even though adaptive optics has been recognized as a promising technology to improve image quality for a large aperture telescope, the question is often asked: "Is adaptive optics needed in a ground-based stellar interferometer?" In this paper, we develop the appropriate theory and provide simulation results to show why adaptive optics is needed in a ground-based optical interferometer. We also present a novel adaptive optics testbed including a tip-tilt error compensation system and a higher-order phase aberration compensation system to verify our theoretical simulation results.

Paper Details

Date Published: 25 August 2005
PDF: 10 pages
Proc. SPIE 5903, Astronomical Adaptive Optics Systems and Applications II, 590305 (25 August 2005); doi: 10.1117/12.614482
Show Author Affiliations
Chueh Ting, New Mexico State Univ. (United States)
Michael K. Giles, New Mexico State Univ. (United States)


Published in SPIE Proceedings Vol. 5903:
Astronomical Adaptive Optics Systems and Applications II
Robert K. Tyson; Michael Lloyd-Hart, Editor(s)

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