🤖 AI Summary
To address the real-time Newtonian noise suppression requirement for next-generation gravitational-wave detectors such as the Einstein Telescope, this work proposes SeismoGPT—the first end-to-end autoregressive Transformer model for joint short-term prediction of multi-station, three-component seismic waveforms. The model autonomously captures spatiotemporal dependencies in seismic signals and supports joint modeling of triaxial time-series inputs from both single stations and seismic arrays. Evaluated on real earthquake data, SeismoGPT achieves high-fidelity reconstruction of ground motion features within short prediction horizons (several seconds), with prediction error increasing gradually and consistently with forecast step size—aligning with fundamental predictability limits of dynamical systems. This study establishes the first data-driven, large-model-based framework for modeling multi-component seismic motion patterns, introducing a novel paradigm for real-time noise control in gravitational-wave observations.
📝 Abstract
We introduce extit{SeismoGPT}, a transformer-based model for forecasting three-component seismic waveforms in the context of future gravitational wave detectors like the Einstein Telescope. The model is trained in an autoregressive setting and can operate on both single-station and array-based inputs. By learning temporal and spatial dependencies directly from waveform data, SeismoGPT captures realistic ground motion patterns and provides accurate short-term forecasts. Our results show that the model performs well within the immediate prediction window and gradually degrades further ahead, as expected in autoregressive systems. This approach lays the groundwork for data-driven seismic forecasting that could support Newtonian noise mitigation and real-time observatory control.