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Globally coherent short duration magnetic field transients and their effect on ground based gravitational-wave detectors

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arxiv 1612.01102 v1 pith:QT7FBU6I submitted 2016-12-04 astro-ph.IM gr-qcphysics.ins-det

classification astro-ph.IMgr-qcphysics.ins-det
keywords magneticdurationgravitational-waveshortdetectorfieldligotransients
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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 $10^{-18}$ 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 2 Pith papers

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score. Full citation record

  1. Correlated magnetic noise from anisotropic lightning sources and the detection of stochastic gravitational waves

    astro-ph.IM 2019-08 conditional novelty 5.0 of 10

    Anisotropic lightning sources do not always worsen Schumann-resonance correlated magnetic noise for stochastic gravitational wave searches, and the Virgo-KAGRA pair is least affected.

  2. A guide to LIGO-Virgo detector noise and extraction of transient gravitational-wave signals

    gr-qc 2019-08 accept novelty 3.0 of 10

    A guide by the LIGO-Virgo collaboration showing that the noise around detected gravitational-wave events is consistent with their models, and that residual correlations vanish when the best-fit waveform is subtracted.

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