Globally coherent short duration magnetic field transients and their effect on ground based gravitational-wave detectors
arXiv:1612.01102 · doi:10.1088/1361-6382/aa60eb
Abstract
It has been recognized that the magnetic fields from the Schumann resonances could affect the search for a stochastic gravitational-wave background by LIGO and Virgo. Presented here are the observations of short duration magnetic field transients that are coincident in the magnetometers at the LIGO and Virgo sites. Data from low-noise magnetometers in Poland and Colorado, USA, are also used and show short duration magnetic transients of global extent. We measure at least 2.3 coincident (between Poland and Colorado) magnetic transient events per day where one of the pulses exceeds 200 pT. Given the recently measured values of the magnetic coupling to differential arm motion for Advanced LIGO, there would be a few events per day that would appear simultaneously at the gravitational-wave detector sites and could move the test masses of order m. We confirm that in the advanced detector era short duration transient gravitational-wave searches must account for correlated magnetic field noise in the global detector network.
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Cited by in corpus (4)
- Parameter estimation with gravitational waves
- A low noise modular current source for stable magnetic field control
- Distinguishing a stochastic gravitational-wave signal from correlated noise with joint parameter estimation: Fisher analysis for ground-based detectors
- Correlation of Gravitational Wave Background Noises and Statistical Loss for Angular Averaged Sensitivity Curves