Three‐dimensional Seismic velocity tomography of Montserrat from the SEA-CALIPSO offshore/onshore experiment

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dc.contributor.author Malin, Peter en
dc.contributor.author Shalev, E en
dc.contributor.author Kenedi, CL en
dc.contributor.author Voight, V en
dc.contributor.author Miller, V en
dc.contributor.author Hidayat, D en
dc.contributor.author Sparks, RS en
dc.contributor.author Minshull, T en
dc.contributor.author Paulatto, M en
dc.contributor.author Brown, L en
dc.contributor.author Mattioli, G en
dc.date.accessioned 2012-03-26T23:01:46Z en
dc.date.issued 2010 en
dc.identifier.citation Geophysical Research Letters 37:7 pages Article number L00E17 2010 en
dc.identifier.issn 0094-8276 en
dc.identifier.uri http://hdl.handle.net/2292/15491 en
dc.description.abstract The Sea-Calipso offshore/onshore experiment was conducted in December 2007 to image the seismic velocity structure of the island of Montserrat. Seismic signals were generated by a towed airgun array at 60 second intervals along a series of circles and radial lines around the island. A total of 4,414 shots were recorded by a network consisting of 204 one-component vertical seismometers in linear deployment, 28 three-component seismometers in a grid deployment, and 10 Ocean Bottom Seismometers (OBS). A first-arrival tomographic inversion covering 45x50 km target area was conducted using the recorded data. In order to avoid a spatial bias, a subset of the data consisting of 58 stations was used. The first-arrival signals were easily identified in most cases. However, in seismic stations deployed close to the shore and/or the volcano, first-arrival signals were less easily identified due to poor signal-to-noise ratio. First-arrival data from 115,158 raypaths were used in a damped smoothed tomographic inversion to produce a 3-dimensional image of the P-seismic velocity to a depth of about 5 km. Inversion results showed areas of high velocity below each of the three volcanic centers of the island at a depth of 2-3 kilometers. Also visible were two areas of low velocity in the northeast and southwest flanks of the island. Modeled land velocities under the island were higher than expected, resulting in raypaths bottoming out at shallower depths without sampling a potential magma chamber at greater depths. en
dc.publisher American Geophysical Union (AGU) en
dc.relation.ispartofseries Geophysical Research Letters en
dc.rights Items in ResearchSpace are protected by copyright, with all rights reserved, unless otherwise indicated. Previously published items are made available in accordance with the copyright policy of the publisher. Details obtained from http://www.sherpa.ac.uk/romeo/issn/0094-8276/ en
dc.rights.uri https://researchspace.auckland.ac.nz/docs/uoa-docs/rights.htm en
dc.title Three‐dimensional Seismic velocity tomography of Montserrat from the SEA-CALIPSO offshore/onshore experiment en
dc.type Journal Article en
dc.identifier.doi 10.1029/2010GL042498 en
pubs.volume 37 en
dc.rights.holder Copyright: American Geophysical Union (AGU) en
dc.rights.accessrights http://purl.org/eprint/accessRights/RestrictedAccess en
pubs.subtype Article en
pubs.elements-id 309577 en
pubs.number L00E17 en
pubs.record-created-at-source-date 2012-03-02 en


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