Paper
1 October 1993 Development and prequalification of a medium-accuracy wide-field pattern recognition starsensor
Peter Verhoeff, Kees de Boom, H. Meier, G. Andre
Author Affiliations +
Abstract
A development of a medium accuracy, CCD based starsensor, intended for use on the new generation of communication satellites is in progress. The sensor aims at an accuracy of 0.06 degree(s) in a FOV of 30 degree(s) X 40 degree(s). The sensor is designed to detect stars with a brightness of mvia <EQ + 2.5 during its whole lifetime of at least 10 years. A breadboard of this starsensor, called Pattern Recognition System (PRS) was built and verified and the manufacturing of an EQM is ongoing now. Intended to be versatile in applications for telecommunication and other missions, a unit is developed which is adaptive and has low recurring cost. The PRS concept is based on new MPP CCD technology. This technology brings passive thermal control without Peltier elements within reach. The electronics accommodated inside the PRS sensorheads is miniaturized by large scale integration by using a Field Programmable Gate Array (FPGA) and Surface Mount Technology (SMT). For cost reasons no microprocessor was implemented. This paper describes the main design features of the PRS, the selection and testing of appropriate CCD, performance characteristics of the system and test results obtained from the PRS breadboard system.
© (1993) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Peter Verhoeff, Kees de Boom, H. Meier, and G. Andre "Development and prequalification of a medium-accuracy wide-field pattern recognition starsensor", Proc. SPIE 1950, Acquisition, Tracking, and Pointing VII, (1 October 1993); https://doi.org/10.1117/12.156606
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Cited by 1 scholarly publication.
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KEYWORDS
Sensors

Charge-coupled devices

Electronics

CCD image sensors

Stars

Video

Clocks

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