Paper
1 July 1992 A radiation-hard, low-background multiplexer design for spacecraft imager applications
Craig O. Staller, Luis Ramirez, Curtiss A. Niblack, Michael A. Blessinger, William E. Kleinhans
Author Affiliations +
Abstract
A possible multiplexer design for the focal plane for the Cassini Visible and Infrared Mapping Spectrometer (VIMS) is reviewed. The instrument's requirements for the multiplexed array are summarized. The VIMS instrument has a modest radiation-hardness requirement due to the trajectory and planetary environments in which the instrument will be required to operate. The total ionizing dose hardness requirement is a few tens of kilorads. A thin-gate oxide of a few hundred angstroms thickness is to be used. Field hardness is to be achieved by guard bands or hardened dielectric isolation. The design is argued to meet the low-noise and radiation-hardness required for imaging at Saturn. The design is versatile enough to provide double-correlated and double-uncorrelated sampling, which is accomplished in the signal processing electronics outside the focal plane.
© (1992) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Craig O. Staller, Luis Ramirez, Curtiss A. Niblack, Michael A. Blessinger, and William E. Kleinhans "A radiation-hard, low-background multiplexer design for spacecraft imager applications", Proc. SPIE 1684, Infrared Readout Electronics, (1 July 1992); https://doi.org/10.1117/12.60506
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Cited by 15 scholarly publications.
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KEYWORDS
Multiplexers

Interference (communication)

Infrared radiation

Electronics

Infrared spectroscopy

Capacitance

Capacitors

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