Impacts of SLR Ground Station Geographic Distribution on Time‐Variable Gravity Recovery

Abstract

Satellite laser ranging (SLR) continues to be an essential technique for estimating Earth’s low‐degree gravity field. GRACE(‐FO) does not accurately recover certain coefficients, which are needed for quantifying large‐scale mass redistribution as part of Earth’s time‐variable gravity (TVG) field. In case of an inter‐mission gap, as with GRACE and GRACE‐FO, SLR can continue to provide mass‐change measurements. The current SLR ground network consists of around 40 stations. However, these are not uniformly distributed and the quantity and quality of data varies widely between sites. We anticipate that future stations will improve SLR‐derived gravity estimates and we investigate their potential impact on the solution in this study. A single new station that enhances network geometry, particularly in the Southern hemisphere, increases the sensitivity of the network by up to 12% for certain coefficients. The addition of 5 new future stations improves certain coefficients up to 18%. We find new stations are limited in their ability to decorrelate certain coefficients regardless of their location, but that adding more data and increasing network uniformity still benefits the overall solution.