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Examination and Enhancement of solar radiation pressure model for BDS-3 satellites
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<p>With the successful launch of the last Geostationary Earth Orbit (GEO) satellite in June 2020, China has completed the construction of the third generation BeiDou navigation satellites system (BDS-3). BDS-3 global services have been initiated in July 2020 with the constellation of 3 GEO, 3 Inclined Geosynchronous Orbit (IGSO) and 24 Medium Earth Orbit (MEO) satellites. In order to further improve the performance of BDS-3 services, the quality of BDS-3 precise orbit product needs further enhancements.</p><p>&#160;&#160;&#160;&#160;&#160;&#160; The solar radiation pressure (SRP) is the main non-conservative orbit perturbation for GNSS satellites and is the key to improve BDS-3 precise orbit determination. In this study, we focus on the SRP models for BDS-3 satellites. Firstly, the widely used Extended CODE Orbit Model with five parameters (ECOM-5) is assessed. With one-year observations of 2020 from both iGMAS and MGEX networks, the five parameters of ECOM model (D0, Y0, B0, Bc and Bs) are estimated for each BDS-3 satellite. The D0 estimates show an obvious dependency on the elevation angle of the Sun above the satellite orbital plane (denoted as &#946;). In addition, large variations can be noticed in eclipse seasons, which indicate the dramatic changes of SRP. The Y0 estimates vary from -0.6 nm/s<sup>2</sup> to 0.6 nm/s<sup>2</sup> for MEO, -1.0 to 1.0 nm/s<sup>2</sup> for IGSO and -1.0 to 1.5 nm/s<sup>2</sup> for GEO satellites. The B0 estimates of several satellites exhibit a clear dependency on the &#946; angle. The largest variation of B0 appears at C45 and C46, changing from 1.0 nm/s<sup>2</sup> at 15 deg to 8.3 nm/s<sup>2</sup> at 64 deg, which implies that the solar panels of these two satellites may have an obvious rotation lag. To compensate the deficiencies of BDS-3 SRP modeling, we introduce several additional parameters into ECOM-5 model (e.g. introducing higher harmonic terms). The POD performances can be improved by about 10% and 40% for BDS-3 MEO/IGSO and GEO satellites, respectively.</p><p>&#160;&#160;&#160;&#160;&#160;&#160; Except for the empirical model, we also study the semi-empirical SRP model such as the a priori box-wing model. Since the geometrical and optical properties from BDS-3 metadata are general and rough, we apply more detailed geometrical and optical coefficients for BDS-3 satellites. The POD performance can be improved by about 10% compared to empirical SRP models. Furthermore, considering Earth radiation pressure will have an impact of about 1.3 cm in radial component for MEO satellites.</p>
Title: Examination and Enhancement of solar radiation pressure model for BDS-3 satellites
Description:
<p>With the successful launch of the last Geostationary Earth Orbit (GEO) satellite in June 2020, China has completed the construction of the third generation BeiDou navigation satellites system (BDS-3).
BDS-3 global services have been initiated in July 2020 with the constellation of 3 GEO, 3 Inclined Geosynchronous Orbit (IGSO) and 24 Medium Earth Orbit (MEO) satellites.
In order to further improve the performance of BDS-3 services, the quality of BDS-3 precise orbit product needs further enhancements.
</p><p>&#160;&#160;&#160;&#160;&#160;&#160; The solar radiation pressure (SRP) is the main non-conservative orbit perturbation for GNSS satellites and is the key to improve BDS-3 precise orbit determination.
In this study, we focus on the SRP models for BDS-3 satellites.
Firstly, the widely used Extended CODE Orbit Model with five parameters (ECOM-5) is assessed.
With one-year observations of 2020 from both iGMAS and MGEX networks, the five parameters of ECOM model (D0, Y0, B0, Bc and Bs) are estimated for each BDS-3 satellite.
The D0 estimates show an obvious dependency on the elevation angle of the Sun above the satellite orbital plane (denoted as &#946;).
In addition, large variations can be noticed in eclipse seasons, which indicate the dramatic changes of SRP.
The Y0 estimates vary from -0.
6 nm/s<sup>2</sup> to 0.
6 nm/s<sup>2</sup> for MEO, -1.
0 to 1.
0 nm/s<sup>2</sup> for IGSO and -1.
0 to 1.
5 nm/s<sup>2</sup> for GEO satellites.
The B0 estimates of several satellites exhibit a clear dependency on the &#946; angle.
The largest variation of B0 appears at C45 and C46, changing from 1.
0 nm/s<sup>2</sup> at 15 deg to 8.
3 nm/s<sup>2</sup> at 64 deg, which implies that the solar panels of these two satellites may have an obvious rotation lag.
To compensate the deficiencies of BDS-3 SRP modeling, we introduce several additional parameters into ECOM-5 model (e.
g.
introducing higher harmonic terms).
The POD performances can be improved by about 10% and 40% for BDS-3 MEO/IGSO and GEO satellites, respectively.
</p><p>&#160;&#160;&#160;&#160;&#160;&#160; Except for the empirical model, we also study the semi-empirical SRP model such as the a priori box-wing model.
Since the geometrical and optical properties from BDS-3 metadata are general and rough, we apply more detailed geometrical and optical coefficients for BDS-3 satellites.
The POD performance can be improved by about 10% compared to empirical SRP models.
Furthermore, considering Earth radiation pressure will have an impact of about 1.
3 cm in radial component for MEO satellites.
</p>.
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