Geophysically Informed Machine Learning for Improving Rapid Estimation and Short‐Term Prediction of Earth Orientation Parameters

Author:

Kiani Shahvandi Mostafa1ORCID,Dill Robert2ORCID,Dobslaw Henryk2ORCID,Kehm Alexander3ORCID,Bloßfeld Mathis3,Schartner Matthias1ORCID,Mishra Siddhartha4,Soja Benedikt1ORCID

Affiliation:

1. Institute of Geodesy and Photogrammetry ETH Zurich Zurich Switzerland

2. Section for Earth System Modelling GFZ German Research Centre for Geosciences Potsdam Germany

3. Deutsches Geodätisches Forschungsinstitut (DGFI‐TUM) Technical University of Munich Munich Germany

4. Seminar for Applied Mathematics Department of Mathematics ETH AI Center ETH Zurich Zurich Switzerland

Abstract

AbstractRapid provision of Earth orientation parameters (EOPs, here polar motion and dUT1) is indispensable in many geodetic applications and also for spacecraft navigation. There are, however, discrepancies between the rapid EOPs and the final EOPs that have a higher latency but the highest accuracy. To reduce these discrepancies, we focus on a data‐driven approach, present a novel method named ResLearner, and use it in the context of deep ensemble learning. Furthermore, we introduce a geophysically constrained approach for ResLearner. We show that the most important geophysical information to improve the rapid EOPs is the effective angular momentum functions of atmosphere, ocean, land hydrology, and sea level. In addition, semidiurnal, diurnal, and long‐period tides coupled with prograde and retrograde tidal excitations are important features. The influence of some climatic indices on the prediction accuracy of dUT1 is discussed, and El Niño Southern Oscillation is found to be influential. We developed an operational framework, providing the improved EOPs on a daily basis with a prediction window of 63 days to fully cover the latency of final EOPs. We show that under the operational conditions and using the rapid EOPs of the International Earth Rotation and Reference Systems Service (IERS), we achieve improvements as high as 60%, thus significantly reducing the differences between rapid and final EOPs. Furthermore, we discuss how the new final series IERS 20 C04 is preferred over 14 C04. Finally, we compare against EOP hindcast experiments of the European Space Agency, on which ResLearner presents comparable improvements.

Publisher

American Geophysical Union (AGU)

Subject

Space and Planetary Science,Earth and Planetary Sciences (miscellaneous),Geochemistry and Petrology,Geophysics

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