Enhanced solar radiation pressure modeling for LEO precise orbit determination: result validation and improvement

Precise orbit knowledge is a fundamental requirement for low Earth orbit (LEO) satellites. Accurate non-gravitational force modeling directly improves the overall quality of LEO precise orbit determination (POD). Time-dependent radiation data and modeled physical effects are considered to address the potential approximation errors in solar radiation pressure (SRP) modeling. We develop an advanced thermal reradiation model for satellite solar panels. A set of improved non-gravitational force models is performed for LEO POD, and we discuss the benefits of the enhanced dynamic models on orbit quality and dependence on empirical parameters. The Gravity Recovery and Climate Experiment Follow-On (GRACE-FO), Jason-3, and Haiyang-2B missions are selected for the POD process. Estimated empirical acceleration and scale parameters and independent satellite laser ranging (SLR) are used to validate the final orbit solutions. The magnitude of empirical acceleration estimated in POD is reduced by 19% with the enhanced dynamic modeling, and the estimated scale factor for the SRP converges to stable and reasonable level. Furthermore, the steady-state temperature model used in thermal reradiation can effectively reduce mismodeled effects in the SRP, and the systematic linear dependency revealed by the SLR residuals is significantly reduced for the GRACE-C and Jason-3 satellites, with improvements of approximately 61% and 49%, respectively. With the enhanced non-gravitational force models, the SLR validation shows the best orbit solutions with RMS values of 10.4, 10.1, 12.4, and 13.2 mm for the GRACE-C, GRACE-D, HY-2B, and Jason-3 satellites, respectively. Overall, advances are made in the explicit modeling of non-gravitational forces to pursue superior satellite orbits, suggesting a more dynamic orbit solution.