Volcano infrasound: progress and future directions

dc.contributor.authorWatson, Leighton M. 
dc.contributor.authorIezzi, Alexandra M. 
dc.contributor.authorToney, Liam 
dc.contributor.authorMaher, Sean P. 
dc.contributor.author Fee, David
dc.contributor.authorMcKee, Kathleen 
dc.contributor.authorOrtiz, Hugo D. 
dc.contributor.authorMatoza, Robin S. 
dc.contributor.authorGestrich, Julia E. 
dc.contributor.authorBishop, Jordan W. 
dc.contributor.authorWitsil, Alex J. C. 
dc.contributor.authorAnderson, Jacob F. 
dc.contributor.authorJohnson, Jefrey B. 
dc.date.accessioned2023-01-11T16:12:42Z
dc.date.available2023-01-11T16:12:42Z
dc.date.issued2022-04-05
dc.description.abstractOver the past two decades (2000–2020), volcano infrasound (acoustic waves with frequencies less than 20 Hz propagating in the atmosphere) has evolved from an area of academic research to a useful monitoring tool. As a result, infrasound is routinely used by volcano observatories around the world to detect, locate, and characterize volcanic activity. It is particularly useful in confrming subaerial activity and monitoring remote eruptions, and it has shown promise in forecasting paroxysmal activity at open-vent systems. Fundamental research on volcano infrasound is providing substantial new insights on eruption dynamics and volcanic processes and will continue to do so over the next decade. The increased availability of infrasound sensors will expand observations of varied eruption styles, and the associated increase in data volume will make machine learning workfows more feasible. More sophisticated modeling will be applied to examine infrasound source and propagation efects from local to global distances, leading to improved infrasound-derived estimates of eruption properties. Future work will use infrasound to detect, locate, and characterize moving fows, such as pyroclastic density currents, lahars, rockfalls, lava fows, and avalanches. Infrasound observations will be further integrated with other data streams, such as seismic, ground- and satellite-based thermal and visual imagery, geodetic, lightning, and gas data. The volcano infrasound community should continue eforts to make data and codes accessible and to improve diversity, equity, and inclusion in the feld. In summary, the next decade of volcano infrasound research will continue to advance our understanding of complex volcano processes through increased data availability, sensor technologies, enhanced modeling capabilities, and novel data analysis methods that will improve hazard detection and mitigation.en_US
dc.description.sponsorshipWe thank two anonymous reviewers and editor Andrew Harris for their constructive comments. This work was partially supported by NSF EAR-1949219 (Watson), NSF EAR-1952392 (Iezzi), NSF EAR-1620576 (Maher), NSF EAR-1847736 (Matoza, Ortiz), NSF EAR-2122188 (Anderson), and NSF EAR-1830976 (Johnson).en_US
dc.description.urihttps://link.springer.com/article/10.1007/s00445-022-01544-wen_US
dc.format.extent13 pagesen_US
dc.genrejournal articlesen_US
dc.identifierdoi:10.13016/m2eo3u-lokb
dc.identifier.citationWatson, L.M., Iezzi, A.M., Toney, L. et al. Volcano infrasound: progress and future directions. Bull Volcanol 84, 44 (2022). https://doi.org/10.1007/s00445-022-01544-wen_US
dc.identifier.urihttps://doi.org/10.1007/s00445-022-01544-w
dc.identifier.urihttp://hdl.handle.net/11603/26622
dc.language.isoen_USen_US
dc.publisherSpringer Natureen_US
dc.relation.isAvailableAtThe University of Maryland, Baltimore County (UMBC)
dc.relation.ispartofUMBC GESTAR II Collection
dc.rightsThis work was written as part of one of the author's official duties as an Employee of the United States Government and is therefore a work of the United States Government. In accordance with 17 U.S.C. 105, no copyright protection is available for such works under U.S. Law.en_US
dc.rightsPublic Domain Mark 1.0*
dc.rights.urihttp://creativecommons.org/publicdomain/mark/1.0/*
dc.titleVolcano infrasound: progress and future directionsen_US
dc.typeTexten_US
dcterms.creatorhttps://orcid.org/0000-0003-3189-9189en_US

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