Paper
6 November 1986 Large Area Space Qualified Thermoelectrically (TE) Cooled HgCdTe MW Photovoltaic Detectors for the Halogen Occultation Experiment (HALOE)
P. W. Norton, P. H. Zimmermann, R. J. Briggs, N. M. Hartle
Author Affiliations +
Abstract
Large area, HgCdTe MW photovoltaic detectors have been developed at Honeywell Electro-Optics Division for the NASA-HALOE instrument. This instrument is scheduled for operation on the Upper Atmospheric Research Satellite (UARS). The photodiodes will be TE cooled and were designed to operate in the 5.1 μm - 5.4 μm band at 185 K to measure Nitric Oxide (NO) concentrations in the atmosphere. To achieve the D* goal of 6 x 109 cm-Hz1/2/W and to meet the spatial responsivity uniformity specification of ± 5% across the 0.6 mm diameter, active area required 15 μm thick devices and a full backside common contact,. Reflections from the backside contact doubled the effective thickness of the detectors. Optical interference from reflections was eliminated with a dual layer front surface A/R coating. Bakeout reliability was optimized by having Au metallization for both n and p interconnects. Detailed performance data and a model for the optical stack are presented.
© (1986) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
P. W. Norton, P. H. Zimmermann, R. J. Briggs, and N. M. Hartle "Large Area Space Qualified Thermoelectrically (TE) Cooled HgCdTe MW Photovoltaic Detectors for the Halogen Occultation Experiment (HALOE)", Proc. SPIE 0686, Infrared Detectors, Sensors, and Focal Plane Arrays, (6 November 1986); https://doi.org/10.1117/12.936536
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Cited by 2 scholarly publications.
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KEYWORDS
Photodiodes

Sensors

Coating

Diffusion

Infrared detectors

Infrared sensors

Mercury cadmium telluride

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