Investigation of magnetic noise in Advanced Virgo
arXiv:1908.11174 · doi:10.1088/1361-6382/ab4974
Abstract
The Advanced Virgo (AdV) sensitivity might be influenced by the effects of environmental noise, in particular magnetic noise (MN). In order to show the impact on the gravitational-wave strain signal h(t) and on the AdV sensitivity, we must understand the coupling between the environmental magnetic activity and the strain. The relationship between the environmental noise - measured by a physical environment monitor (PEM) - and h(t) is investigated using injection studies, where an intentional stimulus is introduced and the responses of both PEM sensors and the instrument are analyzed. We also present the most outstanding measurements and results obtained from both the characterization and the mitigation studies of the environmental MN. Results show that MN does not affect AdV sensitivity up to Mpc in BNS range.
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- A guide to LIGO-Virgo detector noise and extraction of transient gravitational-wave signals
- Site-selection criteria for the Einstein Telescope
- Machine learning for gravitational-wave detection: surrogate Wiener filtering for the prediction and optimized cancellation of Newtonian noise at Virgo
- Stochastic gravitational wave background: methods and Implications
- Impact of Schumann resonances on the Einstein Telescope and projections for the magnetic coupling function
- Correlated 1-1000 Hz magnetic field fluctuations from lightning over earth-scale distances and their impact on gravitational wave searches