Preprints
https://doi.org/10.5194/egusphere-2026-6450
https://doi.org/10.5194/egusphere-2026-6450
03 Nov 2026
 | 03 Nov 2026
Status: this preprint is open for discussion and under review for Ocean Science (OS).

Eulerian space-time statistics of rotational motions from drifters using Gaussian processes

William C. Edge, Matt D. Rayson, Nicole L. Jones, and Lachlan C. Astfalck

Abstract. We applied a Gaussian process regression framework to horizontal velocity data from ocean drifters to infer the space-time scales and total energy of rotational motions in contrasting shelf and ocean regions. A space-time covariance kernel function was chosen to represent rotational motions and its characteristic parameters were inferred directly from the data. We applied the framework to contrasting ocean and shelf environments and found consistent spatial anisotropy in the length scales of each velocity component in both regions, a feature of rotational motion dynamics. The framework resolved rotational features in a macro-tidal shelf environment beyond the limits of nadir altimetry, including a feature with a Rossby number ≈1. The framework estimated time scales in both regions to be less than 10 days, driven by a mix of temporal evolution and low frequency advection. We demonstrate the feasibility of spatiotemporal inference from sparse unstructured oceanographic observations, an approach made tractable using Vecchia's approximation to a Gaussian process, which shows potential for inference studies on large and multi-platform datasets.  

Competing interests: At least one of the (co-)authors is a member of the editorial board of Ocean Science.

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William C. Edge, Matt D. Rayson, Nicole L. Jones, and Lachlan C. Astfalck

Status: open (until 29 Dec 2026)

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William C. Edge, Matt D. Rayson, Nicole L. Jones, and Lachlan C. Astfalck
William C. Edge, Matt D. Rayson, Nicole L. Jones, and Lachlan C. Astfalck
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Short summary
Ocean surface currents evolve in space and time at scales that are difficult to measure in situ. We developed a statistical method that uses floating ocean drifters to characterise the size and time scales of these surface currents. We applied the method to observations from northwestern Australia, on the coastal shelf and in the open ocean. It captured small, fast-evolving eddies on the shelf that are difficult to observe from satellite.
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