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Proceedings Paper

Development of a high-definition IR LED scene projector
Author(s): Dennis T. Norton; Joe LaVeigne; Greg Franks; Steve McHugh; Tony Vengel; Jim Oleson; Michael MacDougal; David Westerfeld
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Paper Abstract

Next-generation Infrared Focal Plane Arrays (IRFPAs) are demonstrating ever increasing frame rates, dynamic range, and format size, while moving to smaller pitch arrays.1 These improvements in IRFPA performance and array format have challenged the IRFPA test community to accurately and reliably test them in a Hardware-In-the-Loop environment utilizing Infrared Scene Projector (IRSP) systems. The rapidly-evolving IR seeker and sensor technology has, in some cases, surpassed the capabilities of existing IRSP technology. To meet the demands of future IRFPA testing, Santa Barbara Infrared Inc. is developing an Infrared Light Emitting Diode IRSP system. Design goals of the system include a peak radiance >2.0W/cm2/sr within the 3.0-5.0μm waveband, maximum frame rates >240Hz, and >4million pixels within a form factor supported by pixel pitches ≤32μm. This paper provides an overview of our current phase of development, system design considerations, and future development work.

Paper Details

Date Published: 3 May 2016
PDF: 7 pages
Proc. SPIE 9820, Infrared Imaging Systems: Design, Analysis, Modeling, and Testing XXVII, 98200X (3 May 2016); doi: 10.1117/12.2225852
Show Author Affiliations
Dennis T. Norton, Santa Barbara Infrared, Inc. (United States)
Joe LaVeigne, Santa Barbara Infrared, Inc. (United States)
Greg Franks, Santa Barbara Infrared, Inc. (United States)
Steve McHugh, Santa Barbara Infrared, Inc. (United States)
Tony Vengel, Santa Barbara Infrared, Inc. (United States)
Jim Oleson, Oleson Convergent Solutions LLC (United States)
Michael MacDougal, Attollo Engineering LLC (United States)
David Westerfeld, Power Photonic Corp. (United States)


Published in SPIE Proceedings Vol. 9820:
Infrared Imaging Systems: Design, Analysis, Modeling, and Testing XXVII
Gerald C. Holst; Keith A. Krapels, Editor(s)

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