Potential of terrestrial reference frame scale transfer using GNSS and SLR co-location onboard LEO satellites

Abstract

Terrestrial scale is one of the key datum parameters in the realization of the International Terrestrial Reference Frame (ITRF), which is defined by Very Long Baseline Interferometry (VLBI) and Satellite Laser Ranging (SLR) in the latest ITRF2020. Currently, the scale of GNSS is aligned to ITRF by estimating phase center offsets (PCOs) of GNSS satellites in a global adjustment with minimum constraints to ITRF. With the proposal of space tie concept in recent years, the co-location of different techniques on the same Low Earth Orbit (LEO) spacecraft provides a possible alternative to achieve this scale datum transfer between different techniques. In this study, we investigate the potential of terrestrial scale transfer between GNSS and SLR using the co-location onboard LEO satellites. The integrated precise orbit determination of GNSS and LEO satellites is performed based on one year of onboard GPS data and SLR observations from GRACE-FO and Swarm satellites as well as a global GNSS network. Two GNSS-only solutions and four GNSS + SLR combined solutions are generated. The results indicate that the scale determined by LEO gravitational constraint in the GNSS-only solution presents an average offset of -0.35 ppb w.r.t. ITRF2020. The space-ties onboard LEO satellites fail to transfer SLR scale information to GNSS network. With the inclusion of SLR observations to LEO satellites, the scale factor of the combined solution is only changed by less than 0.05 ppb with respect to the GNSS-only solution. The small changes of a few millimeters in GPS PCO of the orbital radial direction for the combined solution also demonstrate that the GPS z-PCOs cannot inherit any SLR scale information through LEO co-locations. Meanwhile, we find that the range biases of GRACE-FO and Swarm satellites achieve a good consistency for the majority of SLR stations, since these satellites carry the same type of laser retroreflector arrays and can achieve comparable orbit accuracy. The result indicates that estimating a common range bias parameter is sufficient for GRACE-FO and Swarm when using the SLR observations from these satellites.