Journal of Geodesy

, Volume 92, Issue 2, pp 109–121 | Cite as

An a priori solar radiation pressure model for the QZSS Michibiki satellite

  • Qile Zhao
  • Guo Chen
  • Jing Guo
  • Jingnan Liu
  • Xianglin Liu
Original Article

Abstract

It has been noted that the satellite laser ranging (SLR) residuals of the Quasi-Zenith Satellite System (QZSS) Michibiki satellite orbits show very marked dependence on the elevation angle of the Sun above the orbital plane (i.e., the \(\beta \) angle). It is well recognized that the systematic error is caused by mismodeling of the solar radiation pressure (SRP). Although the error can be reduced by the updated ECOM SRP model, the orbit error is still very large when the satellite switches to orbit-normal (ON) orientation. In this study, an a priori SRP model was established for the QZSS Michibiki satellite to enhance the ECOM model. This model is expressed in ECOM’s D, Y, and B axes (DYB) using seven parameters for the yaw-steering (YS) mode, and additional three parameters are used to compensate the remaining modeling deficiencies, particularly the perturbations in the Y axis, based on a redefined DYB for the ON mode. With the proposed a priori model, QZSS Michibiki’s precise orbits over 21 months were determined. SLR validation indicated that the systematic \(\beta \)-angle-dependent error was reduced when the satellite was in the YS mode, and better than an 8-cm root mean square (RMS) was achieved. More importantly, the orbit quality was also improved significantly when the satellite was in the ON mode. Relative to ECOM and adjustable box-wing model, the proposed SRP model showed the best performance in the ON mode, and the RMS of the SLR residuals was better than 15 cm, which was a two times improvement over the ECOM without a priori model used, but was still two times worse than the YS mode.

Keywords

QZSS Michibiki Solar radiation pressure Precise orbit determination MGEX Yaw-steering attitude Orbit-normal attitude 

Notes

Acknowledgements

The IGS MGEX, iGMAS, and ILRS are greatly acknowledged for providing the multi-GNSS and SLR tracking data. The research is partially supported by the National Natural Science Foundation of China (Grant Nos. 41404032, 41504009, 41574030, 41574027). Finally, the authors are also grateful for the comments and remarks of reviewers and editor-in-chief, who helped to improve the manuscript significantly.

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Copyright information

© Springer-Verlag GmbH Germany 2017

Authors and Affiliations

  1. 1.GNSS Research CenterWuhan UniversityWuhanChina
  2. 2.Collaborative Innovation Center of Geospatial TechnologyWuhan UniversityWuhanChina
  3. 3.School of Geodesy and GeomaticsWuhan UniversityWuhanChina
  4. 4.School of Civil Engineering and GeosciencesNewcastle UniversityNewcastle upon TyneUK
  5. 5.Fugro Intersite B.V.LeidschendamThe Netherlands

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