Potential and scientific requirements of optical clock networks for validating satellite gravity missions
Stefan Schr\"oder, Simon Stellmer, J\"urgen Kusche

TL;DR
This paper explores the potential of using a network of optical clocks across Europe to detect large-scale temporal changes in Earth's gravity field, aiding satellite mission validation.
Contribution
It proposes a novel method of utilizing optical clock networks combined with GNSS data to monitor Earth's geopotential variations over days or weeks.
Findings
Hydrological signals at annual scales can be detected with current clock accuracy.
Atmospheric variations at weekly scales are observable with conservative assumptions.
Clock and GNSS uncertainties still allow effective detection of large-scale geopotential changes.
Abstract
The GRACE and GRACE-FO missions have provided an unprecedented quantification of large-scale changes in the water cycle. However, it is still an open problem of how these missions' data sets can be referenced to a ground truth. Meanwhile, stationary optical clocks show fractional instabilities below when averaged over an hour, and continue to be improved in terms of precision and accuracy, uptime, and transportability. The frequency of a clock is affected by the gravitational redshift, and thus depends on the local geopotential; a relative frequency change of corresponds to a geoid height change of about cm. Here we suggest that this effect could be further exploited for sensing large-scale temporal geopotential changes via a network of clocks distributed at the Earth's surface. In fact, several projects have already proposed to create an ensemble of optical…
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