2019
DOI: 10.1088/1361-6382/ab28c1
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Optimization of seismometer arrays for the cancellation of Newtonian noise from seismic body waves

Abstract: Newtonian noise from seismic fields is predicted to become a sensitivity limiting noise contribution of the gravitational-wave detectors Advanced LIGO and Virgo in the next few years. It also plays a major role in the planning of next-generation detectors, which might be constructed underground, as planned for the Einstein Telescope, mostly to suppress Newtonian noise. Coherent noise cancellation using Wiener filters provides a way to mitigate Newtonian noise. So far, only the cancellation of Newtonian noise p… Show more

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Cited by 42 publications
(77 citation statements)
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“…Rayleigh waves are predicted to give the dominant contribution to NN in surface detectors (Coughlin et al, 2016;Harms et al, 2020), and even underground detectors can still be limited by gravitational noise from Rayleigh waves depending on the detector depth (Badaracco & Harms, 2019). The Rayleigh field produces surface displacement and density perturbations beneath the surface at the same time (Beccaria 10.1029/2020JB020401 et al, 1998Hughes & Thorne, 1998), which leads to gravity perturbations.…”
Section: Resultsmentioning
confidence: 99%
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“…Rayleigh waves are predicted to give the dominant contribution to NN in surface detectors (Coughlin et al, 2016;Harms et al, 2020), and even underground detectors can still be limited by gravitational noise from Rayleigh waves depending on the detector depth (Badaracco & Harms, 2019). The Rayleigh field produces surface displacement and density perturbations beneath the surface at the same time (Beccaria 10.1029/2020JB020401 et al, 1998Hughes & Thorne, 1998), which leads to gravity perturbations.…”
Section: Resultsmentioning
confidence: 99%
“…Another mechanism is by gravitational coupling giving rise to NN and cannot be shielded in any way (Beker et al, 2011(Beker et al, , 2015. A well-explored cancelation scheme is based on Wiener filters (Badaracco & Harms, 2019;Cella, 2000; One of the most important things in NN cancelation is the homogeneity of the seismic field. Scattering of seismic fields from an irregular surface topography can cause heterogeneity of the seismic field.…”
Section: Introductionmentioning
confidence: 99%
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“…Only under near ideal conditions, the required information can be obtained from a single point; see, for example, [22]. Generally, one should expect that many sensors are required [23,24]. Current plans for the Virgo NNcancellation system foresee the deployment of 30 seismometers around each test mass.…”
Section: Introductionmentioning
confidence: 99%
“…The great unsolved problem is how to optimally place sensors to make sure that the information required for NN cancellation is extracted from the field. First optimization results were obtained for simplified models of seismic fields [23,24], but a rigorous optimization based on seismic observations does not exist yet. The scale of this effort is immense, but the sources can be easily monitored as long as they are known, and a major advantage is that the coupling to the detector data is linear, which greatly facilitates noise cancellation.…”
Section: Introductionmentioning
confidence: 99%