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In the site survey of a four-sided traverse, internal angles are essential to ensure geometric accuracy. The survey revealed that the sum of the measured internal angles was 359 degrees and 48 minutes, which is 12 minutes less than the expected 360 degrees. This discrepancy signals an error likely arising from measurement inaccuracies during the fieldwork.To rectify this error, the adjustment process involved distributing the 12-minute shortfall equally across the four internal angles. By...
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Dynamic accuracy measurement method for star trackers using a time-synchronized high-accuracy turntable.

Rui Lu, Jianfu Zhang, Xing Han

    Applied Optics
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    A new method accurately measures star tracker performance under dynamic conditions using a synchronized swing table and real stars. This approach enhances satellite navigation accuracy by providing reliable, on-orbit-like validation.

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    Area of Science:

    • Spacecraft Attitude Determination
    • Navigation Systems Engineering
    • Optical Sensor Metrology

    Background:

    • Star trackers are critical for spacecraft attitude control, providing essential navigation data.
    • Inaccurate attitude information from star trackers can lead to significant navigation errors and mission failure.
    • Ground validation of star tracker accuracy, particularly under dynamic conditions, is challenging.

    Purpose of the Study:

    • To propose and validate a novel method for measuring star tracker accuracy under dynamic conditions.
    • To overcome limitations of ground-based testing for highly dynamic star trackers.
    • To enable comprehensive performance verification, including sensitivity and capture probability.

    Main Methods:

    • Utilized a high-accuracy synchronized swing table to simulate dynamic spacecraft motion.
    • Employed coordinate transformations to predict initial star tracker attitude.
    • Synchronized the swing table, star tracker, and test equipment to minimize systematic errors.
    • Used real navigation stars as targets for measurement, unlike simulated star methods.

    Main Results:

    • The proposed method allows star trackers to maintain tracking at angular velocities up to 20°/s.
    • Achieved more sufficient statistical sample points and reliable results due to continuous tracking.
    • Measurements using real stars closely mimic on-orbit performance.
    • Successfully verified multiple star tracker performance metrics in a single experiment.

    Conclusions:

    • The developed accuracy measurement method is effective for evaluating star trackers under highly dynamic conditions.
    • The test environment closely replicates in-orbit conditions, meeting stringent dynamic performance requirements.
    • This method provides a reliable approach for verifying star tracker accuracy and performance.