Paper
28 August 2015 LWIR pupil imaging and prospects for background compensation
Paul LeVan, Ünal Sakoglu, Mark Stegall, Greg Pierce
Author Affiliations +
Abstract
A previous paper described LWIR Pupil Imaging with a sensitive, low-flux focal plane array, and behavior of this type of system for higher flux operations as understood at the time. We continue this investigation, and report on a more detailed characterization of the system over a broad range of pixel fluxes. This characterization is then shown to enable non-uniformity correction over the flux range, using a standard approach. Since many commercial tracking platforms include a “guider port” that accepts pulse width modulation (PWM) error signals, we have also investigated a variation on the use of this port to “dither” the tracking platform in synchronization with the continuous collection of infrared images. The resulting capability has a broad range of applications that extend from generating scene motion in the laboratory for quantifying performance of “realtime, scene-based non-uniformity correction” approaches, to effectuating subtraction of bright backgrounds by alternating viewing aspect between a point source and adjacent, source-free backgrounds.
© (2015) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Paul LeVan, Ünal Sakoglu, Mark Stegall, and Greg Pierce "LWIR pupil imaging and prospects for background compensation", Proc. SPIE 9609, Infrared Sensors, Devices, and Applications V, 96090U (28 August 2015); https://doi.org/10.1117/12.2190354
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KEYWORDS
Staring arrays

Nonuniformity corrections

Telescopes

Imaging systems

Long wavelength infrared

Infrared imaging

Infrared telescopes

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