Limiting the effects of earthquakes on gravitational-wave interferometers
Michael Coughlin, Paul Earle, Jan Harms, Sebastien Biscans,, Christopher Buchanan, Eric Coughlin, Fred Donovan, Jeremy Fee, Hunter, Gabbard, Michelle Guy, Nikhil Mukund, Matthew Perry

TL;DR
This paper presents an early warning system leveraging real-time earthquake alerts and machine learning to predict and mitigate the impact of seismic events on gravitational-wave detectors, enhancing their operational stability.
Contribution
It introduces a novel earthquake early warning and prediction system specifically designed to protect gravitational-wave interferometers from seismic disruptions.
Findings
90% of ground-motion predictions are within a factor of 5 of actual values
The system can prevent detector interruptions for 40-100 earthquakes over six months
Minimal error when using preliminary earthquake data for predictions
Abstract
Ground-based gravitational wave interferometers such as the Laser Interferometer Gravitational-wave Observatory (LIGO) are susceptible to high-magnitude teleseismic events, which can interrupt their operation in science mode and significantly reduce the duty cycle. It can take several hours for a detector to stabilize enough to return to its nominal state for scientific observations. The down time can be reduced if advance warning of impending shaking is received and the impact is suppressed in the isolation system with the goal of maintaining stable operation even at the expense of increased instrumental noise. Here we describe an early warning system for modern gravitational-wave observatories. The system relies on near real-time earthquake alerts provided by the U.S. Geological Survey (USGS) and the National Oceanic and Atmospheric Administration (NOAA). Hypocenter and magnitude…
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