Reliable star pattern identification technique by using neural networks

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An approach to systematically structuring star patterns and an associated identification technique using a neural network and rule-based expert system is addressed. In stellar-inertial navigation systems based upon modem star trackers, star pattern identification has been characterized primarily as a database search problem. The proposed algorithm herein provides a methodology on how to efficiently construct a mission catalog that reduces the size of original data. Grouping neighboring stars for identification makes it possible to decrease data without noticeable performance degradation. The Radial Basis Function (RBF) well known for generic pattern recognitions is employed as a classifier in the simulation. The neural network-based approach in this study, because of associating the star distribution patterns, turns out to decrease computational time in actual space missions. It also minimizes potential noise effects due to clustering algorithm error and/or CCD pixels. Accuracy and performance of the proposed star identification approach have been examined by simulations using the Bright Star Catalog (BSC) J2000 master catalog.
Publisher
AMER ASTRONAUTICAL SOC
Issue Date
2004
Language
English
Article Type
Article; Proceedings Paper
Keywords

ATTITUDE DETERMINATION; VECTOR OBSERVATIONS; ALGORITHM

Citation

JOURNAL OF THE ASTRONAUTICAL SCIENCES, v.52, no.1-2, pp.239 - 249

ISSN
0021-9142
URI
http://hdl.handle.net/10203/84124
Appears in Collection
AE-Journal Papers(저널논문)
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