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Joint seismic and gravity data inversion to image intra-crustal structures: The Ivrea Geophysical Body along the Val Sesia Profile (Piedmont, Italy)

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    SYSNO ASEP0544667
    Document TypeJ - Journal Article
    R&D Document TypeJournal Article
    Subsidiary JČlánek ve WOS
    TitleJoint seismic and gravity data inversion to image intra-crustal structures: The Ivrea Geophysical Body along the Val Sesia Profile (Piedmont, Italy)
    Author(s) Scarponi, M. (CH)
    Hetényi, G. (CH)
    Plomerová, Jaroslava (GFU-E) ORCID, RID, SAI
    Solarino, S. (IT)
    Baron, L. (CH)
    Petri, B. (FR)
    Article number671412
    Source TitleFrontiers in Earth Science. - : Frontiers Media
    Roč. 9, May (2021)
    Number of pages17 s.
    Publication formOnline - E
    Languageeng - English
    CountryCH - Switzerland
    Keywordsjoint inversion ; seismic receiver functions ; gravity anomalies ; Ivrea Geophysical Body ; Ivrea-Verbano Zone ; continental crust ; intra-crustal structure
    Subject RIVDC - Siesmology, Volcanology, Earth Structure
    OECD categoryVolcanology
    R&D ProjectsLM2015079 GA MŠMT - Ministry of Education, Youth and Sports (MEYS)
    GA21-25710S GA ČR - Czech Science Foundation (CSF)
    Method of publishingOpen access
    Institutional supportGFU-E - RVO:67985530
    UT WOS000659893100001
    EID SCOPUS85107594900
    DOI10.3389/feart.2021.671412
    AnnotationWe present results from a joint inversion of new seismic and recently compiled gravity data to constrain the structure of a prominent geophysical anomaly in the European Alps: the Ivrea Geophysical Body (IGB). We investigate the IGB structure along the West-East oriented Val Sesia profile at higher resolution than previous studies. We deployed 10 broadband seismic stations at 5 km spacing for 27 months, producing a new database of similar to 1000 high-quality seismic receiver functions (RFs). The compiled gravity data yields 1 gravity point every 1-2 km along the profile. We set up an inversion scheme, in which RFs and gravity anomalies jointly constrain the shape and the physical properties of the IGB. We model the IGB's top surface as a single density and shear-wave velocity discontinuity, whose geometry is defined by four, spatially variable nodes between far-field constraints. An iterative algorithm was implemented to efficiently explore the model space, directing the search toward better fitting areas. For each new candidate model, we use the velocity-model structures for both ray-tracing and observed-RFs migration, and for computation and migration of synthetic RFs: the two migrated images are then compared via cross-correlation. Similarly, forward gravity modeling for a 2D density distribution is implemented. The joint inversion performance is the product of the seismic and gravity misfits. The inversion results show the IGB protruding at shallow depths with a horizontal width of similar to 30 km in the western part of the profile. Its shallowest segment reaches either 3-7 or 1-3 km depth below sea-level.
    WorkplaceGeophysical Institute
    ContactHana Krejzlíková, kniha@ig.cas.cz, Tel.: 267 103 028
    Year of Publishing2022
    Electronic addresshttps://www.frontiersin.org/articles/10.3389/feart.2021.671412/full
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