Open AccessObservation angular distance error modeling and matching threshold optimization for terrestrial star tracker
Author(s) -
Zhen Wang,
Jie Jiang,
Guangjun Zhang
Publication year - 2019
Publication title -
optics express
Language(s) - English
Resource type - Journals
SCImago Journal Rank - 1.394
H-Index - 271
ISSN - 1094-4087
DOI - 10.1364/oe.27.033518
Subject(s) - angular diameter , star tracker , physics , angular velocity , matching (statistics) , angular resolution (graph drawing) , optics , stars , observational error , identification (biology) , sky , range (aeronautics) , computer science , astrophysics , mathematics , astronomy , statistics , classical mechanics , botany , materials science , combinatorics , composite material , spacecraft , biology
Observation angular distance error, as the difference between the actual observation angular distance and the reference angular distance, is an important parameter that affects the identification success rate, attitude measurement accuracy, and real-time performance of a terrestrial star tracker. It is the criterion to determine whether stars are identified in star identification but is still unclarified to date. To resolve the problem, the observation angular error model is presented in this work. This model determines the variation range of the observation angular distance error by analyzing the factors of astrometric transformations. Then, the optimal angular distance matching threshold expression for a terrestrial star tracker is presented on the basis of the proposed model for the optimal efficiency in star identification. Numerical simulations and a night sky experiment demonstrate that the differences between the theoretical model, simulation and actual experiment results are less than 0.5'' and thereby validate the reliability of our conclusions.