Please use this identifier to cite or link to this item: http://hdl.handle.net/2122/11673
DC FieldValueLanguage
dc.date.accessioned2018-04-06T09:38:13Zen
dc.date.available2018-04-06T09:38:13Zen
dc.date.issued2016-03-30en
dc.identifier.urihttp://hdl.handle.net/2122/11673en
dc.descriptionThis article has been accepted for publication in Geophysical Journal Internationa ©: The Authors 2016. Published by Oxford University Press on behalf of the Royal Astronomical Society. All rights reserved. Uploaded in accordance with the publisher's self-archiving policy.en
dc.description.abstractWe review the theory of the Earth’s elastic and gravitational response to a surface disk load. The solutions for displacement of the surface and the geoid are developed using expansions of Legendre polynomials, their derivatives and the load Love numbers. We provide a MATLAB function called diskload that computes the solutions for both uncompensated and compensated disk loads. In order to numerically implement the Legendre expansions, it is necessary to choose a harmonic degree, nmax, at which to truncate the series used to construct the solutions. We present a rule of thumb (ROT) for choosing an appropriate value of nmax, describe the consequences of truncating the expansions prematurely and provide a means to judiciously violate the ROT when that becomes a practical necessityen
dc.language.isoEnglishen
dc.relation.ispartofGeophysical Journal Internationalen
dc.relation.ispartofseries/205 (2016)en
dc.titleOn computing the geoelastic response to a disk loaden
dc.typearticleen
dc.description.statusPublisheden
dc.type.QualityControlPeer-revieweden
dc.description.pagenumber1804–1812en
dc.identifier.doi10.1093/gji/ggw115en
dc.description.obiettivoSpecifico7T. Struttura della Terra e geodinamicaen
dc.description.journalTypeJCR Journalen
dc.contributor.authorBevis, Michaelen
dc.contributor.authorMelini, Danieleen
dc.contributor.authorSpada, Giorgioen
dc.contributor.departmentSchool of Earth Sciences, the Ohio State University, Columbus, Ohio, USAen
dc.contributor.departmentIstituto Nazionale di Geofisica e Vulcanologia (INGV), Sezione Roma1, Roma, Italiaen
dc.contributor.departmentDipartimento di Scienze Pure e Applicate (DiSPeA), Università di Urbino, Italyen
item.openairetypearticle-
item.cerifentitytypePublications-
item.languageiso639-1en-
item.grantfulltextopen-
item.openairecristypehttp://purl.org/coar/resource_type/c_18cf-
item.fulltextWith Fulltext-
crisitem.author.deptSchool of Earth Sciences, the Ohio State University, Columbus, Ohio, USA-
crisitem.author.deptIstituto Nazionale di Geofisica e Vulcanologia (INGV), Sezione Roma1, Roma, Italia-
crisitem.author.deptInsitute of Physics, University of Urbino, Italy-
crisitem.author.orcid0000-0002-5383-2375-
crisitem.author.parentorgIstituto Nazionale di Geofisica e Vulcanologia-
crisitem.department.parentorgIstituto Nazionale di Geofisica e Vulcanologia-
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