Paper
15 November 1993 Time-tag photon detection with the MAMA detector system
Giorgio Giaretta, Elliott P. Horch, J. Gethyn Timothy, John F. Heanue, David B. Kasle
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Abstract
The Multi-Anode Microchannel Array (MAMA) detector system is a true photon-counting imager which records the position and arrival time of each detected photon for post facto image reconstruction analysis. Imaging by time-tag photon detection with the MAMA is being used for image stabilization on sounding rockets, and for speckle interferometry and speckle image reconstruction at ground-based telescopes using the Stanford University Speckle Interferometer System (SUSIS). This paper describes the construction and mode-of-operation of the MAMA time-tag photon-detection system, including recent improvements to the data- handling system which permit a data-recording rate in excess of 1 M event s-1. The intrinsic time resolution of the MAMA detector system is < 300 ns and the time resolution of the SUSIS used to date is 3.2 microsecond(s) for each detected photon. A number of examples of both laboratory data and visible-light speckle interferometric deconvolutions and two-dimensional speckle image reconstructions are presented.
© (1993) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Giorgio Giaretta, Elliott P. Horch, J. Gethyn Timothy, John F. Heanue, and David B. Kasle "Time-tag photon detection with the MAMA detector system", Proc. SPIE 1952, Surveillance Technologies and Imaging Components, (15 November 1993); https://doi.org/10.1117/12.161409
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Cited by 1 scholarly publication.
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KEYWORDS
Sensors

Speckle

Stars

Telescopes

Speckle interferometry

Image restoration

Photodetectors

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