CHEN Yuan-zhi, HAO Sheng-guo, HAO Zhi-hang. Method for star identification using connection cluster[J]. Editorial Office of Optics and Precision Engineering, 2000,(3): 217-220
CHEN Yuan-zhi, HAO Sheng-guo, HAO Zhi-hang. Method for star identification using connection cluster[J]. Editorial Office of Optics and Precision Engineering, 2000,(3): 217-220DOI:
The most accurate instrument for satellite attitude determination is star tracker now
in which the key problem is the identification of star map. In this paper
cluster match is performed only with the observed star position information and using the star angular distance between observed star map and guide star catalog
then match identification is made with respect to the connection of the observed star map
at last
utilizing the computer(main frequency 120M)simulation the effects of threshold and position noise on identification and identification time are analyzed. When the threshold is 0.05°
position noise δ is less than 0.02°
in any areas
the identification efficiency is 100%
and the average identification time is less than 0.2s.
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references
Scholl Marija S. Star field identification algorithm-performance verification using simulated star fields[C]. Proc. SPIE, 1993, 2019: 275-290.
DeAntonio L, Udomkesmalee S et al. Star-tracker based autonomous attitude determinction[C]. Proc. SPIE, 1993, 1949: 204-216.
Roelof W H, van Bezooijen. True-sky demonstration of an autonomous star tracker[C]. Proc. SPIE, 1994, 2221: 156-168.