Star image recognition based on mutual star distribution

Di Jiang, Ke Zhang, Olivier Debeir

Research output: Contribution to journalArticlepeer-review

1 Scopus citations

Abstract

A novel method is designed to divide the star image into polygons, in order to solve the problem of setting the grid size in the grid algorithm. Via the method, each star is located in a corresponding polygon. The geometric features of these polygons are extracted and applied for matching the feature patterns of the guidance star database and the observed star image. Simulations indicate that the novel method removes the possible phenomenon in the grid algorithm where more than one star are located in the same grid. The grid algorithm's disadvantage of recognition failure resulting from identifying incorrect close neighbor star for reference star can be overcome and the accuracy of star image recognition is greatly improved.

Original languageEnglish
Pages (from-to)127-131
Number of pages5
JournalXi Tong Gong Cheng Yu Dian Zi Ji Shu/Systems Engineering and Electronics
Volume40
Issue number1
DOIs
StatePublished - 1 Jan 2018

Keywords

  • Feature pattern
  • Perpendicular bisector
  • Polygon
  • Star image recognition

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