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Proceedings Paper

Fringe tracker for the CHARA array
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Paper Abstract

Atmospheric fluctuations cause a jitter in the fringe position of ground-based stellar interferometers. To efficiently use the few photons available, an active fringe tracking system is necessary to stabilize the fringe position. This paper briefly describes the different methods of fringe tracking being implemented at the CHARA array, as well as the fringe tracking systems themselves.

Paper Details

Date Published: 21 February 2003
PDF: 10 pages
Proc. SPIE 4838, Interferometry for Optical Astronomy II, (21 February 2003); doi: 10.1117/12.459323
Show Author Affiliations
Chad E. Ogden, CHARA Array/Mt. Wilson (United States)
Theo Armand ten Brummelaar, CHARA Array/Mt. Wilson (United States)
Judit Sturmann, CHARA Array/Mt. Wilson (United States)

Published in SPIE Proceedings Vol. 4838:
Interferometry for Optical Astronomy II
Wesley A. Traub, Editor(s)

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