Improved kHz-SLR tracking techniques and orbit quality analysis for LEO missions

• Published in: Advances in space research Vol. 45; no. 6; pp. 721 - 732
• Main Authors: Hausleitner, W., Kirchner, G., Krauss, S., Weingrill, J., Pail, R., Goiginger, H., Rieser, D.
• Format: Journal Article
• Language: English
• Published: Oxford Elsevier Ltd 15.03.2010; Elsevier
• Subjects: Astronomy; Earth, ocean, space; Exact sciences and technology; External geophysics; Low earth orbit; Orbit determination; Satellite laser ranging; Orbit determination; Satellite laser ranging; Low earth orbit; Validation; Space remote sensing; Satellite observation; Trajectories; Sea surface temperature; Space research; Optimization; Global Positioning System; Algorithms; System performance; Dynamics; Satellite tracking; Positions; Height; Earth orbit; Visibility; Gravity
• ISSN: 0273-1177; 1879-1948
• DOI: 10.1016/j.asr.2009.11.016

Satellite gravity field missions such as CHAMP, GRACE and GOCE are designed as low Earth orbiting spacecraft (LEO) with orbit heights of about 250–500 km. The challenging mission objectives require a very precise knowledge of the satellite orbit position in space. For these missions precise orbit information is typically provided by GPS satellite-to-satellite tracking (SST) observations supported by satellite laser ranging (SLR). The role of SLR is primarily devoted to serve as an independent tracking instrument used to calibrate and validate the on-board GPS flight receiver. However, the very limited visibility of LEOs from SLR ground stations together with the accordingly high angular rates necessary for the laser mounting to follow the satellite make it more difficult to track LEO missions. At the Observatory Graz–Lustbühel, the Space Research Institute of the Austrian Academy of Sciences operates a very novel SLR facility which was continuously upgraded during the recent years, and is today the only station worldwide capable to operate at kHz-firing rates. The activities presented here focus on a number of hardware upgrades and methodical improvements at the SLR station Graz aiming for a faster and more reliable target acquisition. These include upgrades of laser tracking algorithms as well as a redesign of the laser detection package in particular for LEO spacecraft. These improvements allow an extension of the measurement durations and thus increase the number of observations per pass. As a result we are able to raise the normal point accuracy as well as the overall system performance for LEO tracking. Improvements of the pointing accuracy and the range gate control system lead to a data quantity raise of about 5%. Another task addresses both a geometric and dynamic arc comparison of SLR derived orbits with GPS SST orbit solutions. In the case of CHAMP, the resulting one-way SLR range residuals are in the order of a few centimetres. This allows to draw conclusions on the accuracy of orbit solutions. In order to evaluate the performance of this technique for the upcoming GOCE mission, investigations are carried out in an analogous manner based on simulated GOCE SLR observations. In this study, it is demonstrated that satellite laser ranging, in particular with high-rate tracking capabilities and low orbit optimizations, offers a valuable tool for orbit validation purposes.