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dc.date.accessioned2023-03-13T17:45:18Z
dc.date.available2023-03-13T17:45:18Z
dc.date.created2022-12-08T08:05:25Z
dc.date.issued2022
dc.identifier.citationAbbrescia, M. Avanzini, C. Baldini, L. Ferroli, R. Baldini Batignani, G. Battaglieri, M. Boi, S. Bossini, E. Carnesecchi, F. Casula, M. Cavazza, D. Cicalò, C. Cifarelli, L. Coccetti, F. Coccia, E. Corvaglia, A. Gruttola, D. De Pasquale, S. De Galante, L. Garbini, M. Gemme, G. Gnesi, I. Gramstad, Eirik Grazzi, S. Hatzifotiadou, D. Rocca, P. La Liu, Z. Lombardo, L. Mandaglio, G. Margotti, A. Maron, G. Mazziotta, M.N. Mazzola, M. Mulliri, A. Nania, R. Noferini, F. Nozzoli, F. Ould-Saada, Farid Palmonari, F. Panareo, M. Panetta, M.P. Paoletti, R. Parvis, M. Pellegrino, C. Perasso, L. Pinazza, O. Pinto, C. Pisano, S. Riggi, F. Righini, G. Ripoli, C. Rizzi, M. Sartorelli, G. Scapparone, E. Schioppa, M. Scioli, G. Scribano, A. Selvi, M. Taiuti, M. Terreni, G. Trifirò, A. Trimarchi, M. Viola, A.P. Vistoli, C. Håland, Even Simonsen Votano, L. Williams, M.C.S. Zichichi, A. Zuyeuski, R. . Observation of Rayleigh-Lamb waves generated by the 2022 Hunga-Tonga volcanic eruption with the POLA detectors at Ny-Ålesund. Scientific Reports. 2022, 12(1)
dc.identifier.urihttp://hdl.handle.net/10852/101403
dc.description.abstractThe eruption of the Hunga-Tonga volcano in the South Pacific Ocean on January 15, 2022, at about 4:15 UTC, generated a violent explosion, which created atmospheric pressure disturbances in the form of Rayleigh-Lamb waves detected all over the globe. Here we discuss the observation of the Hunga-Tonga shock-wave performed at the Ny-Ålesund Research Station on the Spitsbergen island, by the detectors of the PolarquEEEst experiment and their ancillary sensors. Online pressure data as well as the results of dedicated offline analysis are presented and discussed in details. Results include wave arrival times, wave amplitude measurements and wave velocity calculation. We observed five passages of the shock wave with a significance larger than 3 σ and an amplitude up to 1 hPa. The average propagation velocity resulted to be (308 ± 0.6) m/s. Possible effects of the atmospheric pressure variation associated with the shock-wave multiple passages on the cosmic-ray rate at ground level are also investigated. We did not find any significant evidence of this effect.
dc.languageEN
dc.publisherNature Portfolio
dc.rightsAttribution 4.0 International
dc.rights.urihttps://creativecommons.org/licenses/by/4.0/
dc.titleObservation of Rayleigh-Lamb waves generated by the 2022 Hunga-Tonga volcanic eruption with the POLA detectors at Ny-Ålesund
dc.title.alternativeENEngelskEnglishObservation of Rayleigh-Lamb waves generated by the 2022 Hunga-Tonga volcanic eruption with the POLA detectors at Ny-Ålesund
dc.typeJournal article
dc.creator.authorAbbrescia, M.
dc.creator.authorAvanzini, C.
dc.creator.authorBaldini, L.
dc.creator.authorFerroli, R. Baldini
dc.creator.authorBatignani, G.
dc.creator.authorBattaglieri, M.
dc.creator.authorBoi, S.
dc.creator.authorBossini, E.
dc.creator.authorCarnesecchi, F.
dc.creator.authorCasula, M.
dc.creator.authorCavazza, D.
dc.creator.authorCicalò, C.
dc.creator.authorCifarelli, L.
dc.creator.authorCoccetti, F.
dc.creator.authorCoccia, E.
dc.creator.authorCorvaglia, A.
dc.creator.authorGruttola, D. De
dc.creator.authorPasquale, S. De
dc.creator.authorGalante, L.
dc.creator.authorGarbini, M.
dc.creator.authorGemme, G.
dc.creator.authorGnesi, I.
dc.creator.authorGramstad, Eirik
dc.creator.authorGrazzi, S.
dc.creator.authorHatzifotiadou, D.
dc.creator.authorRocca, P. La
dc.creator.authorLiu, Z.
dc.creator.authorLombardo, L.
dc.creator.authorMandaglio, G.
dc.creator.authorMargotti, A.
dc.creator.authorMaron, G.
dc.creator.authorMazziotta, M.N.
dc.creator.authorMazzola, M.
dc.creator.authorMulliri, A.
dc.creator.authorNania, R.
dc.creator.authorNoferini, F.
dc.creator.authorNozzoli, F.
dc.creator.authorOuld-Saada, Farid
dc.creator.authorPalmonari, F.
dc.creator.authorPanareo, M.
dc.creator.authorPanetta, M.P.
dc.creator.authorPaoletti, R.
dc.creator.authorParvis, M.
dc.creator.authorPellegrino, C.
dc.creator.authorPerasso, L.
dc.creator.authorPinazza, O.
dc.creator.authorPinto, C.
dc.creator.authorPisano, S.
dc.creator.authorRiggi, F.
dc.creator.authorRighini, G.
dc.creator.authorRipoli, C.
dc.creator.authorRizzi, M.
dc.creator.authorSartorelli, G.
dc.creator.authorScapparone, E.
dc.creator.authorSchioppa, M.
dc.creator.authorScioli, G.
dc.creator.authorScribano, A.
dc.creator.authorSelvi, M.
dc.creator.authorTaiuti, M.
dc.creator.authorTerreni, G.
dc.creator.authorTrifirò, A.
dc.creator.authorTrimarchi, M.
dc.creator.authorViola, A.P.
dc.creator.authorVistoli, C.
dc.creator.authorHåland, Even Simonsen
dc.creator.authorVotano, L.
dc.creator.authorWilliams, M.C.S.
dc.creator.authorZichichi, A.
dc.creator.authorZuyeuski, R.
cristin.unitcode185,15,4,60
cristin.unitnameHøyenergifysikk
cristin.ispublishedtrue
cristin.fulltextoriginal
cristin.qualitycode1
dc.identifier.cristin2090406
dc.identifier.bibliographiccitationinfo:ofi/fmt:kev:mtx:ctx&ctx_ver=Z39.88-2004&rft_val_fmt=info:ofi/fmt:kev:mtx:journal&rft.jtitle=Scientific Reports&rft.volume=12&rft.spage=&rft.date=2022
dc.identifier.jtitleScientific Reports
dc.identifier.volume12
dc.identifier.issue1
dc.identifier.pagecount0
dc.identifier.doihttps://doi.org/10.1038/s41598-022-23984-2
dc.type.documentTidsskriftartikkel
dc.type.peerreviewedPeer reviewed
dc.source.issn2045-2322
dc.type.versionPublishedVersion
cristin.articleid19978


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