TY - JOUR
T1 - Perceiving the Crust in 3-D
T2 - A Model Integrating Geological, Geochemical, and Geophysical Data
AU - Strati, Virginia
AU - Wipperfurth, Scott A.
AU - Baldoncini, Marica
AU - McDonough, William F.
AU - Mantovani, Fabio
N1 - Funding Information:
This work was partially funded by the National Institute of Nuclear Physics (INFN) through the ITALian RADioactivity project (ITALRAD) and by the Theoretical Astroparticle Physics (TAsP) research network. The coauthors acknowledge the support of the Geological and Seismic Survey of the Umbria Region (UMBRIARAD), the University of Ferrara (Fondo di Ateneo per la Ricerca scientifica FAR 2016), the Project Agroalimentare Idrointelligente CUP D92I16000030009 and the MIUR (Ministero dell’Istruzione, dell’Università e della Ricerca) under MIUR-PRIN-2012 project. S. A. Wipperfurth gratefully acknowledges support from the support of DOE-INFN exchange program (2016) and the UMD GS Summer Research Fellowship. W.F. McDonough gratefully acknowledges support from NSF EAR 1067983, the University of Maryland, and Tohoku University. The authors thank Ivan Callegari, Kassandra Raptis, Matteo Albèri, Giovanni Fiorentini, Barbara Ricci, Gerti Xhixha, Enrico Chiarelli, Carlo Bottardi Barbara Ricci, Gerti Xhixha, Enrico for useful discussions. Richard Ash for help with the ICPMS analyses. The authors are grateful to Oladele Olaniyan and Richard Smith for providing help and sharing data of the 3-D model published in Olaniyan et al. (2015). The authors appreciate the essential support and valuable insights from Mike Easton, Mark Chen, Nigel Smith, Eligio Lisi and Pedro Jugo. Finally, we appreciate and thank the careful reviews from J. C. Mareschal and an anonymous reviewer, and insights from and editorial efforts of Uli Faul. Readers can find detailed geochemistry data and the 3-D numerical model in supporting information. Author contributions: Virginia Strati, Fabio Mantovani, and William McDonough conceived and designed the work as it is. Virginia Strati and Scott Wipperfurth carried out the sampling survey and together with Marica Baldoncini performed the Th and U analyses with HPGe detectors. Scott Wipperfurth carried out the ICPMS measurements. The 3-D geophysical model was constructed by Virginia Strati and Fabio Mantovani. All the authors participated in the data analysis and interpretation of the results, while Virginia Strati, Marica Baldoncini, Fabio Mantovani conducted the geoneutrino signal calculation. Virginia Strati, Fabio Mantovani took the lead in designing and composing the manuscript with the input from all the authors. All the authors critically revised and provided final approval of the version submitted.
Publisher Copyright:
© 2017. American Geophysical Union. All Rights Reserved.
PY - 2017/12
Y1 - 2017/12
N2 - Regional characterization of the continental crust has classically been performed through either geologic mapping, geochemical sampling, or geophysical surveys. Rarely are these techniques fully integrated, due to limits of data coverage, quality, and/or incompatible data sets. We combine geologic observations, geochemical sampling, and geophysical surveys to create a coherent 3-D geologic model of a 50 × 50 km upper crustal region surrounding the SNOLAB underground physics laboratory in Canada, which includes the Southern Province, the Superior Province, the Sudbury Structure, and the Grenville Front Tectonic Zone. Nine representative aggregate units of exposed lithologies are geologically characterized, geophysically constrained, and probed with 109 rock samples supported by compiled geochemical databases. A detailed study of the lognormal distributions of U and Th abundances and of their correlation permits a bivariate analysis for a robust treatment of the uncertainties. A downloadable 3-D numerical model of U and Th distribution defines an average heat production of 1.5+1.4-0.7 µW/m3, and predicts a contribution of 7.7+7.7-3.0 TNU (a Terrestrial Neutrino Unit is one geoneutrino event per 1032 target protons per year) out of a crustal geoneutrino signal of 31.1+8.0-4.5 TNU. The relatively high local crust geoneutrino signal together with its large variability strongly restrict the SNO+ capability of experimentally discriminating among BSE compositional models of the mantle. Future work to constrain the crustal heat production and the geoneutrino signal at SNO+ will be inefficient without more detailed geophysical characterization of the 3-D structure of the heterogeneous Huronian Supergroup, which contributes the largest uncertainty to the calculation.
AB - Regional characterization of the continental crust has classically been performed through either geologic mapping, geochemical sampling, or geophysical surveys. Rarely are these techniques fully integrated, due to limits of data coverage, quality, and/or incompatible data sets. We combine geologic observations, geochemical sampling, and geophysical surveys to create a coherent 3-D geologic model of a 50 × 50 km upper crustal region surrounding the SNOLAB underground physics laboratory in Canada, which includes the Southern Province, the Superior Province, the Sudbury Structure, and the Grenville Front Tectonic Zone. Nine representative aggregate units of exposed lithologies are geologically characterized, geophysically constrained, and probed with 109 rock samples supported by compiled geochemical databases. A detailed study of the lognormal distributions of U and Th abundances and of their correlation permits a bivariate analysis for a robust treatment of the uncertainties. A downloadable 3-D numerical model of U and Th distribution defines an average heat production of 1.5+1.4-0.7 µW/m3, and predicts a contribution of 7.7+7.7-3.0 TNU (a Terrestrial Neutrino Unit is one geoneutrino event per 1032 target protons per year) out of a crustal geoneutrino signal of 31.1+8.0-4.5 TNU. The relatively high local crust geoneutrino signal together with its large variability strongly restrict the SNO+ capability of experimentally discriminating among BSE compositional models of the mantle. Future work to constrain the crustal heat production and the geoneutrino signal at SNO+ will be inefficient without more detailed geophysical characterization of the 3-D structure of the heterogeneous Huronian Supergroup, which contributes the largest uncertainty to the calculation.
KW - 3-D modeling
KW - SNO+
KW - continental lithosphere
KW - geoneutrinos
KW - radiogenic heat production
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U2 - 10.1002/2017GC007067
DO - 10.1002/2017GC007067
M3 - Article
AN - SCOPUS:85036591644
SN - 1525-2027
VL - 18
SP - 4326
EP - 4341
JO - Geochemistry, Geophysics, Geosystems
JF - Geochemistry, Geophysics, Geosystems
IS - 12
ER -