Clock synchronization and light-travel-time estimation for space-based gravitational-wave detectors
Jan Niklas Reinhardt, Olaf Hartwig, and Gerhard Heinzel

TL;DR
This paper presents an accurate pseudorange model and a novel Kalman filter algorithm for clock synchronization and light-travel-time estimation in space-based gravitational-wave detectors, achieving submeter accuracy essential for data processing.
Contribution
It introduces a realistic pseudorange model in the barycentric reference frame and a specialized Kalman filter algorithm to disentangle pseudoranges and synchronize clocks in space-based GW detectors.
Findings
Achieves submeter accuracy in clock synchronization and light-travel-time estimation.
Provides a realistic pseudorange model for space-based GW detectors.
Demonstrates the effectiveness of the proposed algorithm with data simulations.
Abstract
Space-based gravitational-wave detectors, such as LISA, record interferometric measurements on widely separated satellites. Their clocks are not synced actively. Instead, clock synchronization is performed in on-ground data processing. It relies on measurements of the so-called pseudoranges, which entangle the interspacecraft light travel times with the clock desynchronizations between emitting and receiving spacecraft. For interspacecraft clock synchronization, we need to isolate the differential clock desynchronizations, i.e., disentangle the pseudoranges. This further yields estimates for the interspacecraft light travel times, which are required as delays for the laser frequency noise suppression via time-delay interferometry. Previous studies on pseudorange disentanglement apply various simplifications in the pseudorange modeling and the data simulation. In contrast, this article…
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Taxonomy
TopicsAdvanced Frequency and Time Standards · Geophysics and Sensor Technology · Atomic and Subatomic Physics Research
