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Proceedings Paper

Optimal SNR exposure time for speckle imaging: experimental results with frequency-dependent detector noise
Author(s): David W. Tyler; Andrew H. Suzuki; Mark A. Von Bokern; Donna D. B. Keating; Michael C. Roggemann
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Paper Abstract

We review recent arguments for using increased spectral bandwidth and exposure times to optimize the signal-to-noise ratio of speckle imaging estimators and discuss the tradeoff between camera exposure time and the number of data frames collected when observing time is fixed. We compare experimental results with a previously-derived expression for optimal exposure time and find reasonable agreement after accounting for frequency-dependent camera noise.

Paper Details

Date Published: 1 June 1994
PDF: 9 pages
Proc. SPIE 2198, Instrumentation in Astronomy VIII, (1 June 1994); doi: 10.1117/12.176694
Show Author Affiliations
David W. Tyler, Air Force Phillips Lab. (United States)
Andrew H. Suzuki, Air Force Phillips Lab. (United States)
Mark A. Von Bokern, Air Force Phillips Lab. (United States)
Donna D. B. Keating, Air Force Phillips Lab. (United States)
Michael C. Roggemann, Air Force Institute of Technology (United States)


Published in SPIE Proceedings Vol. 2198:
Instrumentation in Astronomy VIII
David L. Crawford; Eric R. Craine, Editor(s)

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