An Empirical Solar Radiation Pressure Model for Autonomous GNSS Orbit Prediction

J. Ala-Luhtala, M. Seppänen, and R. Piché

Abstract:	GNSS satellite orbits can be predicted by integrating the satellites’ equation of motion. If the prediction is done in a consumer grade positioning device, a simplified version of the equation of motion is required. The forces due to Earth’s gravitation, solar gravitation and lunar gravitation should be included, but the models for the smaller non-gravitational forces can be fairly simple. This paper presents a simple empirical two parameter solar radiation pressure model for an orbit prediction application in a navigation device that does not have a network connection. The model is tested by predicting the orbits of GPS and GLONASS satellites up to 5 days into the future, using position and improved velocity from broadcast ephemerides as an initial state. The predicted orbits are compared to the precise orbits from International GNSS Service (IGS).
Published in:	Proceedings of IEEE/ION PLANS 2012 April 24 - 26, 2012 Myrtle Beach Marriott Resort & Spa Myrtle Beach, South Carolina
Pages:	568 - 575
Cite this article:	Ala-Luhtala, J., Seppänen, M., Piché, R., "An Empirical Solar Radiation Pressure Model for Autonomous GNSS Orbit Prediction," Proceedings of IEEE/ION PLANS 2012, Myrtle Beach, South Carolina , April 2012, pp. 568-575. https://doi.org/10.1109/PLANS.2012.6236929
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