广播星历 Resources

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This document details the computation of satellite positions in the Earth-Centered Earth-Fixed (ECEF) coordinate system. The process involves calculating Keplerian orbital parameters using Kepler's equation based on the 21 broadcast ephemeris parameters, followed by determining satellite coordinates through kinematic equations. Implementation is demonstrated using MATLAB R2011b to read satellite navigation (O, N) files, with detailed explanations of the program workflow, key functions, and annotated code segments for coordinate calculation.

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