Towards the 1 mm/y Stability of the Radial Orbit Error at Regional Scales

• Published in: Advances in space research Vol. 55; no. 1
• Main Authors: Couhert, Alexandre, Cerri, Luca, Legeais, Jean-Francois, Ablain, Michael, Zelensky, Nikita P., Haines, Bruce J., Lemoine, Frank G., Bertiger, William I., Desai, Shailen D., Otten, Michiel
• Format: Journal Article
• Language: English
• Published: Goddard Space Flight Center Science Direct 01-01-2015
• Subjects: Geosciences (General); Space Sciences (General); Satellite Altimetry; Precision Orbit Determination (pod); Jason
• ISSN: 0273-1177
• DOI: 10.1016/j.asr.2014.06.041

An estimated orbit error budget for the Jason-1 and Jason-2 GDR-D solutions is constructed, using several measures of orbit error. The focus is on the long-term stability of the orbit time series for mean sea level applications on a regional scale. We discuss various issues related to the assessment of radial orbit error trends; in particular this study reviews orbit errors dependent on the tracking technique, with an aim to monitoring the long-term stability of all available tracking systems operating on Jason-1 and Jason-2 (GPS, DORIS, SLR). The reference frame accuracy and its effect on Jason orbit is assessed. We also examine the impact of analysis method on the inference of Geographically Correlated Errors as well as the significance of estimated radial orbit error trends versus the time span of the analysis. Thus a long-term error budget of the 10-year Jason-1 and Envisat GDR-D orbit time series is provided for two time scales: interannual and decadal. As the temporal variations of the geopotential remain one of the primary limitations in the Precision Orbit Determination modeling, the overall accuracy of the Jason-1 and Jason-2 GDR-D solutions is evaluated through comparison with external orbits based on different time-variable gravity models. This contribution is limited to an East-West "order-1" pattern at the 2 mm/y level (secular) and 4 mm level (seasonal), over the Jason-2 lifetime. The possibility of achieving sub-mm/y radial orbit stability over interannual and decadal periods at regional scales and the challenge of evaluating such an improvement using in situ independent data is discussed.