NASA Logo

NTRS

NTRS - NASA Technical Reports Server

Press Enter or click the Search button to begin your search.

Back to Results
Gallium arsenide quantum well-based far infrared array radiometric imagerWe have built an array-based camera (FIRARI) for thermal imaging (lambda = 8 to 12 microns). FIRARI uses a square format 128 by 128 element array of aluminum gallium arsenide quantum well detectors that are indium bump bonded to a high capacity silicon multiplexer. The quantum well detectors offer good responsivity along with high response and noise uniformity, resulting in excellent thermal images without compensation for variation in pixel response. A noise equivalent temperature difference of 0.02 K at a scene temperature of 290 K was achieved with the array operating at 60 K. FIRARI demonstrated that AlGaAS quantum well detector technology can provide large format arrays with performance superior to mercury cadmium telluride at far less cost.
Document ID
19920013209
Acquisition Source
Legacy CDMS
Document Type
Conference Paper
Authors
Forrest, Kathrine A.
(NASA Goddard Space Flight Center Greenbelt, MD, United States)
Jhabvala, Murzy D.
(NASA Goddard Space Flight Center Greenbelt, MD, United States)
Date Acquired
September 6, 2013
Publication Date
December 1, 1991
Publication Information
Publication: NASA, Washington, Technology 2001: The Second National Technology Transfer Conference and Exposition, Volume 1
Subject Category
Instrumentation And Photography
Accession Number
92N22452
Distribution Limits
Public
Copyright
Work of the US Gov. Public Use Permitted.
No Preview Available