Proceedings Paper
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Paper Abstract
A six-feature, all-sky star field identification algorithm has been developed for autonomous navigation. The minimum identifiable star pattern element consists of an ordered star triplet defined by three stars and their celestial coordinates (right ascension and declination). The star field identification algorithm was integrated with the CCD-based star tracker and tested at the Table Mountain Observatory. Real-time star field identification is reported with a CCD-based imaging camera interfaced to SPARC II workstation.
Paper Details
Date Published: 1 October 1993
PDF: 7 pages
Proc. SPIE 2019, Infrared Spaceborne Remote Sensing, (1 October 1993); doi: 10.1117/12.157849
Published in SPIE Proceedings Vol. 2019:
Infrared Spaceborne Remote Sensing
Marija S. Scholl, Editor(s)
PDF: 7 pages
Proc. SPIE 2019, Infrared Spaceborne Remote Sensing, (1 October 1993); doi: 10.1117/12.157849
Show Author Affiliations
Marija S. Scholl, Alenka Associates (United States)
Published in SPIE Proceedings Vol. 2019:
Infrared Spaceborne Remote Sensing
Marija S. Scholl, Editor(s)
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