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Journal Article
Published: 01 October 2021
Italian Journal of Geosciences (2021) 140 (3): 365–381.
..., are evaluated from literature suggestions ( C aterino et alii , 2018 ). Finally, with reference to the case study of the “San Benedetto” school of Norcia (Central Italy), the proposed methodology is satisfactorily verified by comparing the forecast with real costs. The innovative aspect of the proposed...
FIGURES | View All (21)
Journal Article
Published: 07 September 2021
Bulletin of the Seismological Society of America (2022) 112 (1): 262–286.
...Arben Pitarka; Aybige Akinci; Pasquale De Gori; Mauro Buttinelli ABSTRACT The M w 6.5 Norcia, Italy, earthquake occurred on 30 October 2016 and caused extensive damage to buildings in the epicentral area. The earthquake was recorded by a network of strong‐motion stations, including 14 stations...
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Journal Article
Journal: Geology
Published: 01 June 2020
Geology (2020) 48 (9): 924–928.
... similar preparatory phases in nature remains difficult because it requires dense monitoring in advance. The 2016 Amatrice-Visso-Norcia (central Italy) earthquake cascade, captured by an unprecedented seismic network, provided a unique testing ground to image the preparatory phase of a large event...
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Journal Article
Journal: Geophysics
Published: 23 June 2022
Geophysics (2022) 87 (4): WB55–WB67.
... , including the conventionally processed profile (Figure  5a ) and the two raw deconvolved profiles (Figure  5b and 5c , spiking and Gabor, respectively). Table 1. Acquisition parameters of the 3D GPR data volume collected at the Castelluccio di Norcia Basin in Central Italy (after Ercoli et al...
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Journal Article
Published: 27 December 2018
Seismological Research Letters (2019) 90 (2A): 659–671.
... from near‐source records. The method, based on a piecewise linear detrend of the strong‐motion (SM) recordings, is applied to reconstruct the ground displacement field of the 30 October 2016 M w 6.5 earthquake in central Italy. The robustness of the results is checked against geodetic measurements...
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Journal Article
Published: 20 September 2024
Bulletin of the Seismological Society of America (2024) 114 (6): 2912–2925.
... seismic events affecting the Italian territory is tested using the 2016 Norcia, Italy, earthquake showing the method reconstruction capabilities, its robustness to noise and to network geometry changes, and its real‐time potential. The most widely used approach to generate ground‐shaking maps...
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Journal Article
Published: 11 April 2018
Seismological Research Letters (2018) 89 (3): 1118–1128.
... the application of this scheme to sequences that either conform, or do not, to the MOL behavior, such as the Amatrice–Norcia (Italy 2016–2017), Emilia (Italy 2012), and Tohoku‐Oki (Japan 2011) aftershock sequences. © Seismological Society of America To make more quantitative evaluations, we define three...
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Image
Illustration of the doughnut effect for (a) the 7 November 2016 M 5 Cushing, Oklahoma, earthquake and (b) the 30 October 2016 M 6.6 Norcia, Italy, earthquake. For the Cushing earthquake, the maximum “Did You Feel It?” (DYFI) intensity is of 6.7 at 5.5 km of the epicenter (see Data and Resources). The maximum DYFI intensity is 9 in Norcia for the eponym earthquake (see Data and Resources). There were no application launches nor felt reports collected within 10 min and 15 km of the Cushing epicenter (a), this gap being filled after 10 min. For the damaging Norcia earthquake, within the same time and distance windows, only one damaging felt report was collected. No other felt reports were collected within 15 km of the epicenter, despite several late (i.e., after 10 min) application launches. Only observations collected within 1 hr of the earthquakes are presented.
Published: 06 December 2017
Figure 8. Illustration of the doughnut effect for (a) the 7 November 2016 M  5 Cushing, Oklahoma, earthquake and (b) the 30 October 2016 M  6.6 Norcia, Italy, earthquake. For the Cushing earthquake, the maximum “Did You Feel It?” (DYFI) intensity is of 6.7 at 5.5 km of the epicenter (see Data
Image
Displacement waveforms processed with eBASCO (black lines) and NESS2 standard algorithm (gray lines) plotted along with Global Positioning System (GPS; squares) coseismic displacement values (left panels). On the right panels, the related displacement spectra are shown with their identification code: (a) event EMSC‐20161030_0000029 30 October 2016 Norcia (Italy; CLO station); (b) event IT‐2009‐0009 6 April 2009 L’Aquila (Italy; AQV station); and (c) event USGS‐us20005iis 15 April 2016 Kumamoto (Japan; KMM18 station). DS, Displacement Spectra; EMSC, European‐Mediterranean Seismological Centre; USGS, U.S. Geological Survey.
Published: 29 June 2021
with their identification code: (a) event EMSC‐20161030_0000029 30 October 2016 Norcia (Italy; CLO station); (b) event IT‐2009‐0009 6 April 2009 L’Aquila (Italy; AQV station); and (c) event USGS‐us20005iis 15 April 2016 Kumamoto (Japan; KMM18 station). DS, Displacement Spectra; EMSC, European‐Mediterranean Seismological
Image
Examples of acceleration and velocity waveforms exhibiting evidence of near‐source effects. Station code and component orientation are reported together with the moment magnitude Mw and the rupture distance RRUP. PGA and PGV values are also listed. (a) Pulse‐like velocity traces recorded at IT.ACC station (2016 Mw 6.5 Norcia, Italy, event) and BO.SMN01 station (2000 Mw 6.6 Tottori, Japan, earthquake) and wavelet representation (Baker, 2007) of the velocity pulse (black thick line); (b) velocity traces (fault‐normal components) recorded at two stations, BO.KMM15 and BO.KMM19, that were found in diametrically opposed positions with respect to the fault rupture of the 2016 Mw 7.0 Kumamoto‐shi event (Japan); (c) vertical acceleration components recorded at station IT.MRN during the Mw 6.0 second shock of the 2012 Emilia sequence and at IV.T1214 station during the 2016 Mw 6.5 Norcia event; (d) fault‐normal horizontal acceleration component recorded at NZ.WTMC station during the 2016 Mw 8.0 Kaikōura earthquake (New Zealand) and vertical acceleration component recorded at BO.IWT33 station during the 2008 Mw 8.0 Iwate earthquake (Japan).
Published: 03 October 2018
velocity traces recorded at IT.ACC station (2016 M w  6.5 Norcia, Italy, event) and BO.SMN01 station (2000 M w  6.6 Tottori, Japan, earthquake) and wavelet representation ( Baker, 2007 ) of the velocity pulse (black thick line); (b) velocity traces (fault‐normal components) recorded at two
Image
RRSM event page (see Data and Resources) for the Norcia (Central Italy) earthquake that occurred on 30 October 2016 at 06:40:18 UTC. There are 121 triaxial station recordings of this event in the RRSM database; the “List of Stations” in the screenshot—ordered by decreasing peak ground acceleration (PGA)—shows only three of them, all pertaining to the IV network (INGV, 2006). Similar pages are available for all of the earthquakes included in the RRSM database. The color version of this figure is available only in the electronic edition.
Published: 17 February 2021
Figure 2. RRSM event page (see Data and Resources ) for the Norcia (Central Italy) earthquake that occurred on 30 October 2016 at 06:40:18 UTC. There are 121 triaxial station recordings of this event in the RRSM database; the “List of Stations” in the screenshot—ordered by decreasing peak ground
Image
ESM “Event” webpage of the Mw 6.5 Norcia (Central Italy) earthquake (see Data and Resources). The color version of this figure is available only in the electronic edition.
Published: 17 February 2021
Figure 5. ESM “Event” webpage of the M w  6.5 Norcia (Central Italy) earthquake (see Data and Resources ). The color version of this figure is available only in the electronic edition.
Image
Velocity (Vp left panels, Vp/Vs right panels) along the Norcia fault, Italy, (trace in Fig. 1A) with snapshots at different times before the largest earthquake: (A) 13 September 2016 (first fully resolved image), (B) 26 October (before Mw 5.5 shock) and (C) 30 October (before main shock). Black lines indicate similarly well-resolved volumes. Yellow star is Mw 6.5 hypocenter, and white stars are Mw >5.5 earthquakes on 24 August and 26 October. Bottom panel shows velocity on the fault plane right before the event; coseismic slip by Scognamiglio et al. (2018) is plotted to highlight ruptured asperity.
Published: 01 June 2020
Figure 2. Velocity (Vp left panels, Vp/Vs right panels) along the Norcia fault, Italy, (trace in Fig. 1A ) with snapshots at different times before the largest earthquake: (A) 13 September 2016 (first fully resolved image), (B) 26 October (before Mw 5.5 shock) and (C) 30 October (before main
Image
Velocity (Vp top panels, Vp/Vs lower panels) across the Norcia fault, Italy, (traces in Fig. 1A) with snapshots at different times before largest earthquake: (A) 13 September 2016, (B) 26 October, and (C) 30 October (before main shock). Purple lines indicate similarly well-resolved volumes. Black star is Mw 6.5 hypocenter.
Published: 01 June 2020
Figure 3. Velocity (Vp top panels, Vp/Vs lower panels) across the Norcia fault, Italy, (traces in Fig. 1A ) with snapshots at different times before largest earthquake: (A) 13 September 2016, (B) 26 October, and (C) 30 October (before main shock). Purple lines indicate similarly well-resolved
Journal Article
Published: 25 October 2022
Bulletin of the Seismological Society of America (2022) 112 (6): 3037–3045.
..., namely the Amatrice ( M w 6.0) of 24 August 2016 and the Norcia ( M w 6.5) of 30 October 2016 earthquakes. For this analysis, we used seismograms from the central Italy dense seismic array stations, and earthquakes located at hypocenter distances r < 80 km, having magnitudes M w 3.4–6.5. The dataset...
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Journal Article
Published: 01 November 2018
Earthquake Spectra (2018) 34 (4): 1671–1691.
... in Norcia. Reinforced-Concrete (RC) structures in Italy are typically found outside of the historical parts of town and represent the relatively modern inventory of residential buildings. Several RC buildings in Norcia were evacuated after the 24 August Amatrice earthquake. Their vulnerability...
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Journal Article
Journal: GSA Bulletin
Published: 14 December 2020
GSA Bulletin (2021) 133 (7-8): 1679–1694.
... may be better understood considering the recent results on rupture directivity provided by Calderoni et al. (2017) for sixteen earthquakes of Mw > 4.4 belonging to the 2016 Amatrice-Norcia-Visso seismic sequences. The seismic sequences that occurred in the last decades in central Italy...
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Journal Article
Published: 12 November 2019
Bulletin of the Seismological Society of America (2019) 109 (6): 2738–2740.
...) argue that the negative uplift volume associated with the 2016 Amatrice–Norcia, central Italy, earthquake sequence requires a coseismic volume collapse of the hanging wall. Using results for dip‐slip dislocations in an elastic half‐space we show that V uplift = ( P / 4 ) ( 1 − 2 ν ) sin ( 2 δ...
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Typical streets within historical centers of Italy: (a) Santo Stefano di Sessanio, L’Aquila and (b) Norcia, Perugia.
Published: 01 November 2024
Figure 1. Typical streets within historical centers of Italy: (a) Santo Stefano di Sessanio, L’Aquila and (b) Norcia, Perugia.
Image
(A) Map of distribution of earthquakes during 2016–2017 Central Italy seismic sequence (Tan et al., 2021). Stars highlight main-shock epicenters. Lines show traces of major regional faults. (B) Evolution of basement seismic rate (depth &gt;9 km) during sequence (Eqs—earthquakes). Vertical lines mark occurrences of main shocks: A—Amatrice; V—Visso; N—Norcia; C—Campotosto. (C) Plan view at depth of 10 km showing Coulomb stress change (see SM1 [text footnote 1]) and aftershocks (from 10 to 11 km) of Norcia main shock within 30 days. Black rectangle is Norcia main shock fault box.
Published: 14 August 2023
Figure 1. (A) Map of distribution of earthquakes during 2016–2017 Central Italy seismic sequence ( Tan et al., 2021 ). Stars highlight main-shock epicenters. Lines show traces of major regional faults. (B) Evolution of basement seismic rate (depth >9 km) during sequence (Eqs—earthquakes