Abstract A closed-loop integrated model including micro-vibration disturbance, dynamic characteristics of satellite, optical system of star sensor and attitude control algorithm is established. The control torque error caused by additional disturbance torque and the star sensor imaging error caused by structural resonance is fully integrated analyzed, which are firstly presented into the attitude control system (ACS). Steady-state and transient response analyses are completed to evaluate the impact of such two errors on performances of (ACS). Steady-state response results show that the effect of control torque error appears in lower frequency band with a peak of 6.784E-8″ at 53 Hz, while influence of star sensor imaging error on attitude determination mainly concentrates in high frequency band with maximum response of 0.4101″ at 315 Hz. Transient response results show that the two errors will not significantly affect control indicators such as rise time, overshoot and peak time. The results indicate that the influence of star sensor imaging error is non-negligible for satellite ACS which required milli-arc-second attitude control accuracy. According to the analytical results, traditional analysis only on payload optical axis cannot reveal the whole impact of micro vibration on LOS error, the two errors of micro-vibration introduced to ACS in this work must be considered for the development of spacecraft with 0.1″ pointing accuracy.

    Highlights A closed-loop integrated model and attitude control algorithm is established. ACS offset caused by control torque error and star sensor imaging error induced by micro vibration are presented. The two errors significantly affect control indicators under steady-state response condition. Control torque error appears in lower frequency band with small magnitude. Star sensor imaging error mainly concentrates in high frequency band with considerable magnitude.


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    Titel :

    Modeling and analysis of the influence caused by micro-vibration on satellite attitude control system


    Beteiligte:
    Li, Lin (Autor:in) / Yu, Yang (Autor:in) / Wang, Li (Autor:in) / Yuan, Li (Autor:in) / Zhang, Lei (Autor:in) / Gong, Xiaoxue (Autor:in) / Wu, Yanpeng (Autor:in) / Zheng, Ran (Autor:in)

    Erschienen in:

    Acta Astronautica ; 213 ; 71-80


    Erscheinungsdatum :

    2023-08-31


    Format / Umfang :

    10 pages




    Medientyp :

    Aufsatz (Zeitschrift)


    Format :

    Elektronische Ressource


    Sprache :

    Englisch




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