Articles | Volume 33, issue 2
https://doi.org/10.5194/sd-33-173-2024
© Author(s) 2024. This work is distributed under
the Creative Commons Attribution 4.0 License.
the Creative Commons Attribution 4.0 License.
https://doi.org/10.5194/sd-33-173-2024
© Author(s) 2024. This work is distributed under
the Creative Commons Attribution 4.0 License.
the Creative Commons Attribution 4.0 License.
Science report
| 
24 Jun 2024
Science report |
| 24 Jun 2024
| 24 Jun 2024
A strainmeter array as the fulcrum of novel observatory sites along the Alto Tiberina Near Fault Observatory
Lauro Chiaraluce
Istituto Nazionale di Geofisica e Vulcanologia INGV, Rome, Italy
Richard Bennett
Department of Geosciences, University of Arizona UA, Tucson, Arizona, USA
David Mencin
EarthScope Consortium, Boulder, Colorado, USA
Wade Johnson
EarthScope Consortium, Boulder, Colorado, USA
Massimiliano Rinaldo Barchi
Dipartimento di Fisica e Geologia, Università degli Studi di Perugia, Perugia, Italy
Marco Bohnhoff
Geomechanics & Scientific Drilling, GFZ German Research Centre for Geosciences, Telegrafenberg, 14473 Potsdam, Germany
Paola Baccheschi
Istituto Nazionale di Geofisica e Vulcanologia INGV, Rome, Italy
Antonio Caracausi
Istituto Nazionale di Geofisica e Vulcanologia INGV, Palermo, Italy
Carlo Calamita
Istituto Nazionale di Geofisica e Vulcanologia INGV, Ancona, Italy
Adriano Cavaliere
Istituto Nazionale di Geofisica e Vulcanologia INGV, Bologna, Italy
Adriano Gualandi
Istituto Nazionale di Geofisica e Vulcanologia INGV, Rome, Italy
Eugenio Mandler
Istituto Nazionale di Geofisica e Vulcanologia INGV, Bologna, Italy
Maria Teresa Mariucci
Istituto Nazionale di Geofisica e Vulcanologia INGV, Rome, Italy
Leonardo Martelli
Istituto Nazionale di Geofisica e Vulcanologia INGV, Bologna, Italy
Simone Marzorati
Istituto Nazionale di Geofisica e Vulcanologia INGV, Ancona, Italy
Paola Montone
Istituto Nazionale di Geofisica e Vulcanologia INGV, Rome, Italy
Debora Pantaleo
Istituto Nazionale di Geofisica e Vulcanologia INGV, Ancona, Italy
Stefano Pucci
Istituto Nazionale di Geofisica e Vulcanologia INGV, Rome, Italy
Enrico Serpelloni
Istituto Nazionale di Geofisica e Vulcanologia INGV, Bologna, Italy
Istituto Nazionale di Geofisica e Vulcanologia INGV, Rome, Italy
Salvatore Stramondo
Istituto Nazionale di Geofisica e Vulcanologia INGV, Rome, Italy
Catherine Hanagan
Department of Geosciences, University of Arizona UA, Tucson, Arizona, USA
EarthScope Consortium, Boulder, Colorado, USA
Liz Van Boskirk
EarthScope Consortium, Boulder, Colorado, USA
Mike Gottlieb
EarthScope Consortium, Boulder, Colorado, USA
Glen Mattioli
EarthScope Consortium, Boulder, Colorado, USA
Dipartimento di Fisica e Geologia, Università degli Studi di Perugia, Perugia, Italy
Marco Urbani
Dipartimento di Fisica e Geologia, Università degli Studi di Perugia, Perugia, Italy
Francesco Mirabella
Dipartimento di Fisica e Geologia, Università degli Studi di Perugia, Perugia, Italy
Assel Akimbekova
Dipartimento di Fisica e Geologia, Università degli Studi di Perugia, Perugia, Italy
Simona Pierdominici
Geomechanics & Scientific Drilling, GFZ German Research Centre for Geosciences, Telegrafenberg, 14473 Potsdam, Germany
Thomas Wiersberg
Geomechanics & Scientific Drilling, GFZ German Research Centre for Geosciences, Telegrafenberg, 14473 Potsdam, Germany
Chris Marone
Dipartimento di Scienze della Terra, La Sapienza, Università degli Studi Roma, Rome, Italy
Luca Palmieri
Dipartimento di Ingegneria dell'informazione, Università degli Studi di Padova, Padova, Italy
Luca Schenato
Dipartimento di Ingegneria dell'informazione, Università degli Studi di Padova, Padova, Italy
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The STAR project set out to drill six shallow holes and use geophysical logging to find the best depth for placing seismometers and strainmeters to image the upper crust, in particular the Alto Tiberina fault, Italy. These measurements give us a better idea of what the rocks are like, helping us connect what we know from the literature with what we find underground, giving solid information on rock properties, which helps us understand the first few hundred meters of the Earth's crust.
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The STAR project set out to drill six shallow holes and use geophysical logging to find the best depth for placing seismometers and strainmeters to image the upper crust, in particular the Alto Tiberina fault, Italy. These measurements give us a better idea of what the rocks are like, helping us connect what we know from the literature with what we find underground, giving solid information on rock properties, which helps us understand the first few hundred meters of the Earth's crust.
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Tomáš Fischer, Pavla Hrubcová, Torsten Dahm, Heiko Woith, Tomáš Vylita, Matthias Ohrnberger, Josef Vlček, Josef Horálek, Petr Dědeček, Martin Zimmer, Martin P. Lipus, Simona Pierdominici, Jens Kallmeyer, Frank Krüger, Katrin Hannemann, Michael Korn, Horst Kämpf, Thomas Reinsch, Jakub Klicpera, Daniel Vollmer, and Kyriaki Daskalopoulou
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Stefano Gori, Emanuela Falcucci, Chiara Ladina, Simone Marzorati, and Fabrizio Galadini
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Aladino Govoni, Luciana Bonatto, Marco Capello, Adriano Cavaliere, Claudio Chiarabba, Ezio D'Alema, Stefania Danesi, Sara Lovati, Lucia Margheriti, Marco Massa, Salvatore Mazza, Francesco Mazzarini, Stephen Monna, Milena Moretti, Anna Nardi, Davide Piccinini, Claudia Piromallo, Silvia Pondrelli, Simone Salimbeni, Enrico Serpelloni, Stefano Solarino, Massimiliano Vallocchia, Marco Santulin, and the AlpArray Working Group
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We describe here the contribution of Istituto Nazionale di Geofisica e Vulcanolgia (INGV) to the AlpArray Seismic Network (AASN) in the framework of the AlpArray project (http://www.alparray.ethz.ch), a large European collaborative research initiative.
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Luigi Vadacca, Emanuele Casarotti, Lauro Chiaraluce, and Massimo Cocco
Solid Earth, 7, 1537–1549, https://doi.org/10.5194/se-7-1537-2016, https://doi.org/10.5194/se-7-1537-2016, 2016
G. Bossi, M. Cavalli, S. Crema, S. Frigerio, B. Quan Luna, M. Mantovani, G. Marcato, L. Schenato, and A. Pasuto
Nat. Hazards Earth Syst. Sci., 15, 715–722, https://doi.org/10.5194/nhess-15-715-2015, https://doi.org/10.5194/nhess-15-715-2015, 2015
A. Piscini, M. Picchiani, M. Chini, S. Corradini, L. Merucci, F. Del Frate, and S. Stramondo
Atmos. Meas. Tech., 7, 4023–4047, https://doi.org/10.5194/amt-7-4023-2014, https://doi.org/10.5194/amt-7-4023-2014, 2014
V. J. Cortes Arevalo, M. Charrière, G. Bossi, S. Frigerio, L. Schenato, T. Bogaard, C. Bianchizza, A. Pasuto, and S. Sterlacchini
Nat. Hazards Earth Syst. Sci., 14, 2681–2698, https://doi.org/10.5194/nhess-14-2681-2014, https://doi.org/10.5194/nhess-14-2681-2014, 2014
L. Chiaraluce, C. Collettini, M. Cattaneo, and G. Monachesi
Sci. Dril., 17, 31–35, https://doi.org/10.5194/sd-17-31-2014, https://doi.org/10.5194/sd-17-31-2014, 2014
Related subject area
Location/Setting: Instrumentation and observatories | Subject: Geophysics/Seismology | Geoprocesses: Tectonic processes
ICDP drilling of the Eger Rift observatory: magmatic fluids driving the earthquake swarms and deep biosphere
The shallow boreholes at The AltotiBerina near fault Observatory (TABOO; northern Apennines of Italy)
Tomáš Fischer, Pavla Hrubcová, Torsten Dahm, Heiko Woith, Tomáš Vylita, Matthias Ohrnberger, Josef Vlček, Josef Horálek, Petr Dědeček, Martin Zimmer, Martin P. Lipus, Simona Pierdominici, Jens Kallmeyer, Frank Krüger, Katrin Hannemann, Michael Korn, Horst Kämpf, Thomas Reinsch, Jakub Klicpera, Daniel Vollmer, and Kyriaki Daskalopoulou
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Short summary
Short summary
The newly established geodynamic laboratory aims to develop modern, comprehensive, multiparameter observations at depth for studying earthquake swarms, crustal fluid flow, mantle-derived fluid degassing and processes of the deep biosphere. It is located in the West Bohemia–Vogtland (western Eger Rift) geodynamic region and comprises a set of five shallow boreholes with high-frequency 3-D seismic arrays as well as continuous real-time fluid monitoring at depth and the study of the deep biosphere.
L. Chiaraluce, C. Collettini, M. Cattaneo, and G. Monachesi
Sci. Dril., 17, 31–35, https://doi.org/10.5194/sd-17-31-2014, https://doi.org/10.5194/sd-17-31-2014, 2014
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Short summary
We built six observatory stations in central Italy to monitor a fault potentially capable of generating a strong earthquake. Each site has 80–160 m deep wells equipped with strainmeters and seismometers. At the surface, we placed GNSS antennas and seismic and meteorological sensors. All data, which are open access for the scientific community, will help us to better understand the complex physical and chemical processes that lead to the generation of the full range of slow and fast earthquakes.
We built six observatory stations in central Italy to monitor a fault potentially capable of...
