[en] A system was recently implemented in the Virgo detector to cancel noise in its data produced by seismic waves directly coupling with the suspended test masses through gravitational interaction. The data from seismometers are being filtered to produce a coherent estimate of the associated gravitational noise also known as Newtonian noise. The first implementation of the system uses a time-invariant (static) Wiener filter, which is the optimal filter for Newtonian-noise cancellation assuming that the noise is stationary. However, time variations in the form of transients and slow changes in correlations between sensors are possible and while time-variant filters are expected to cope with these variations better than a static Wiener filter, the question is what the limitations are of time-variant noise cancellation. In this study, we present a framework to study the performance limitations of time-variant noise cancellation filters and carry out a proof of concept with adaptive filters on seismic data at the Virgo site. We demonstrate that the adaptive filters, at least those with superior architecture, indeed significantly outperform the static Wiener filter with the residual noise remaining above the statistical error bound.
Disciplines :
Physics
Author, co-author :
Koley, Soumen ; Université de Liège - ULiège > Département d'astrophysique, géophysique et océanographie (AGO) > Ondes gravitationnelles ; Gran Sasso Science Institute (GSSI), L'Aquila, Italy ; INFN, Laboratori Nazionali Del Gran Sasso, Assergi, Italy
Harms, Jan; Gran Sasso Science Institute (GSSI), L'Aquila, Italy ; INFN, Laboratori Nazionali Del Gran Sasso, Assergi, Italy
Allocca, Annalisa; Università di Napoli Federico II, Napoli, Italy ; INFN, Sezione di Napoli, Napoli, Italy
Calloni, Enrico; Università di Napoli Federico II, Napoli, Italy ; INFN, Sezione di Napoli, Napoli, Italy
De Rosa, Rosario; Università di Napoli Federico II, Napoli, Italy ; INFN, Sezione di Napoli, Napoli, Italy
Errico, Luciano; Università di Napoli Federico II, Napoli, Italy ; INFN, Sezione di Napoli, Napoli, Italy
Esposito, Marina; Università di Napoli Federico II, Napoli, Italy ; INFN, Sezione di Napoli, Napoli, Italy
Badaracco, Francesca; INFN, Sezione di Genova, Genova, Italy
Rei, Luca; INFN, Sezione di Genova, Genova, Italy
Bertolini, Alessandro; INFN, Sezione di Napoli, Napoli, Italy
Cieslar, Marek; Astronomical Observatory, University of Warsaw, Warsaw, Poland ; Nicolaus Copernicus Astronomical Center, Polish Academy of Sciences, Warsaw, Poland
Pietrzak, Mateusz; Astronomical Observatory, University of Warsaw, Warsaw, Poland ; Nicolaus Copernicus Astronomical Center, Polish Academy of Sciences, Warsaw, Poland
Suchenek, Mariusz; Astronomical Observatory, University of Warsaw, Warsaw, Poland ; Nicolaus Copernicus Astronomical Center, Polish Academy of Sciences, Warsaw, Poland
Fiori, Irene; European Gravitational Observatory (EGO), Pisa, Italy
Paoli, Andrea; European Gravitational Observatory (EGO), Pisa, Italy
Tringali, Maria Concetta; European Gravitational Observatory (EGO), Pisa, Italy
Ruggi, Paolo; European Gravitational Observatory (EGO), Pisa, Italy
Istituto Nazionale di Fisica Nucleare Sezione di Padova CNRS - Centre National de la Recherche Scientifique NWO - Nederlandse Organisatie voor Wetenschappelijk Onderzoek AEI - Agencia Estatal de Investigación Generalitat Valenciana Generalitat de Catalunya NCN - Narodowe Centrum Nauki ERDF - European Regional Development Fund OTKA - Hungarian Scientific Research Fund F.R.S.-FNRS - Fonds de la Recherche Scientifique FWO - Fonds Wetenschappelijk Onderzoek Vlaanderen EC - European Commission NSF - National Science Foundation STFC - Science and Technology Facilities Council MIUR - Ministero dell'Istruzione, dell'Università e della Ricerca
Funding text :
The authors gratefully acknowledge the Italian Istituto Nazionale di Fisica Nucleare (INFN), the French Centre National de la Recherche Scientifique (CNRS) and the Netherlands Organization for Scientific Research (NWO), for the construction and operation of the Virgo detector and the creation and support of the EGO consortium. The authors also gratefully acknowledge research support from these agencies as well as by the Spanish Agencia Estatal de Investigaci\u00F3n, the Consellera d\u2019Innovaci\u00F3, Universitats, Ci\u00E8ncia i Societat Digital de la Generalitat Valenciana and the CERCA Programme Generalitat de Catalunya, Spain, the National Science Centre of Poland and the European Union-European Regional Development Fund; Foundation for Polish Science (FNP), the Hungarian Scientific Research Fund (OTKA), the French Lyon Institute of Origins (LIO), the Belgian Fonds de la Recherche Scientifique (FRS-FNRS), Actions de Recherche Concert\u00E9es (ARC) and Fonds Wetenschappelijk Onderzoek-Vlaanderen (FWO), Belgium, the European Commission. The authors gratefully acknowledge the support of the NSF, STFC, INFN, CNRS, and Nikhef for provision of computational resources. S.\u2009K. acknowledges the support through a collaboration agreement between Gran Sasso Science Institute and Nikhef and from the European Gravitational Observatory through a collaboration convention on Advanced Virgo . The authors also gratefully acknowledge the support of the Italian Ministry of Education, University and Research within the PRIN 2017 Research Program Framework, No. 2017SYRTCN.
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