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Proceedings Paper

Interferometric imaging of geostationary satellites: signal-to-noise considerations
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Paper Abstract

Geostationary satellites are generally too small to image at high resolution with conventional single-dish tele- scopes. An alternative to a 100+ m diameter telescope is to use an optical/infrared interferometer consisting of multiple smaller telescopes in an array configuration. In this paper we focus on what is required to achieve the required signal-to-noise ratio to image. We will look at the signal-to-noise ratio required to track fringes on satellites on multiple baselines, a pre-requisite to imaging.We will also look at how to achieve the required signal- to-noise required for image reconstruction. We compare these performance specifications to the performance of existing interferometers as well as that of a new interferometer concept optimized for satellite imaging.

Paper Details

Date Published: 12 September 2012
PDF: 6 pages
Proc. SPIE 8445, Optical and Infrared Interferometry III, 84452M (12 September 2012); doi: 10.1117/12.925953
Show Author Affiliations
A. M. Jorgensen, New Mexico Institute of Mining and Technology (United States)
H. Schmitt, Computational Physics, Inc. (United States)
U.S. Naval Research Lab. (United States)
D. Mozurkewich, Seabrook Engineering (United States)
J. T. Armstrong, U.S. Naval Research Lab. (United States)
S. Restaino, U.S. Naval Research Lab. (United States)
R. Hindsley, U.S. Naval Research Lab. (United States)


Published in SPIE Proceedings Vol. 8445:
Optical and Infrared Interferometry III
Françoise Delplancke; Jayadev K. Rajagopal; Fabien Malbet, Editor(s)

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