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Liu, Dongzhu, Su, Xing, Xie, Xin, Zhou, Han, and Qu, Zhengjian, 2025. Study on the Design of Broadcast Ephemeris Parameters for Low Earth Orbit Satellites. Remote Sensing, 17(16):2894, doi:10.3390/rs17162894.
• from the NASA Astrophysics Data System • by the DOI System •
@ARTICLE{2025RemS...17.2894L,
       author = {{Liu}, Dongzhu and {Su}, Xing and {Xie}, Xin and {Zhou}, Han and {Qu}, Zhengjian},
        title = "{Study on the Design of Broadcast Ephemeris Parameters for Low Earth Orbit Satellites}",
      journal = {Remote Sensing},
     keywords = {LEO satellite navigation, broadcast ephemeris, Kepler ephemeris model, least squares estimation, ephemeris message size, GNSS},
         year = 2025,
        month = aug,
       volume = {17},
       number = {16},
          eid = {2894},
        pages = {2894},
     abstract = "{The integration of low Earth orbit (LEO) satellite constellations into
        the Global Navigation Satellite System (GNSS) has emerged as a
        prominent research focus, as LEO satellites can significantly
        enhance the precision of GNSS positioning, navigation, and
        timing (PNT) services. In the design of LEO navigation
        constellations, the development of an efficient broadcast
        ephemeris model is critical for delivering high-accuracy
        navigation solutions. This study extends the conventional
        16-parameter Keplerian broadcast ephemeris model by proposing
        enhanced 18-, 20-, 22-, and 24-parameter models, ensuring
        compatibility with existing GNSS ephemeris standards. The
        performance of these models was evaluated using precise science
        orbit from five satellites at varying altitudes, ranging from
        320 km to 1336 km. By analyzing fitting errors, Signal-in-Space
        Range Error (SISRE), and Message Size Bits (MSB) across
        different fitting arc durations and parameter counts, the
        optimal model configuration was identified. The results
        demonstrate that the 22-parameter model, which was constructed
        by augmenting the standard 16-parameter ephemeris with (aË, nË,
        Crs3, Crc3, Crs1, Crc1) delivers the best balance of accuracy
        and efficiency. With a fitting arc length of 20 min, the SISRE
        for the GRACE-A (320 km), GRACE-C (475 km), Sentinel-2A (786
        km), HY-2A (966 km), and Sentinel-6A (1336 km) satellites were
        measured at 8.88 cm, 6.21 cm, 2.87 cm, 2.11 cm, and 0.75 cm,
        respectively. Meanwhile, the corresponding MSB remained compact
        at 501, 490, 491, 487, and 476 bits. These findings confirm that
        the proposed 22-parameter broadcast ephemeris model meets the
        stringent accuracy requirements for next-generation LEO-
        augmented GNSSs, paving the way for enhanced global navigation
        services.}",
          doi = {10.3390/rs17162894},
       adsurl = {https://ui.adsabs.harvard.edu/abs/2025RemS...17.2894L},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}
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