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arxiv: 1611.04683 · v1 · pith:HB4GWVEYnew · submitted 2016-11-15 · 🌌 astro-ph.IM · cs.IT· math.IT

Real-time kinematic positioning of LEO satellites using a single-frequency GPS receiver

classification 🌌 astro-ph.IM cs.ITmath.IT
keywords kinematicmethodpositioningreal-timesingle-frequencyaccuracydeterminationorbit
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Due to their low cost and low power consumption, single-frequency GPS receivers are considered suitable for low-cost space applications such as small satellite missions. Recently, requirements have emerged for real-time accurate orbit determination at sub-meter level in order to carry out onboard geocoding of high-resolution imagery, open-loop operation of altimeters and radio occultation. This study proposes an improved real-time kinematic positioning method for LEO satellites using single-frequency receivers. The C/A code and L1 phase are combined to eliminate ionospheric effects. The epoch-differenced carrier phase measurements are utilized to acquire receiver position changes which are further used to smooth the absolute positions. A kinematic Kalman filter is developed to implement kinematic orbit determination. Actual flight data from China small satellite SJ-9A are used to test the navigation performance. Results show that the proposed method outperforms traditional kinematic positioning method in terms of accuracy. A 3D position accuracy of 0.72 m and 0.79 m has been achieved using the predicted portion of IGS ultra-rapid products and broadcast ephemerides, respectively.

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