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  • 1
    ISSN: 1573-157X
    Keywords: ground ruptures ; Italy ; seismotectonics ; Umbria-Marche earthquakes
    Source: Springer Online Journal Archives 1860-2000
    Topics: Geosciences , Physics
    Notes: Abstract We classified the most outstanding rupturesof the 1997 Umbria-Marche seismic sequence assecondary tectonic effects that occur within the zoneof deformation induced by the deep displacement on theseismogenic structure. The trend of the surfacedeformation is homogeneous within the entire area ofinterest and consistent with NE-oriented extensionevidenced by CMT focal solutions of the three mainshocks. We extrapolate the discontinuous sites ofbreak measurements and suggest that the localdeformation concentrates along four narrow bands.Location and direction of these bands are locallycontrolled by pre-existing structures. The comparisonbetween our data with the seismological data – such asmain rupture planes and spatial aftershockdistribution – highlights that three bands mark partof the boundaries of the NW-SE elongated aftershocksarea and the fourth occurs where this area is widest.Moreover, the analysis of the structural setting ofthe area suggests that N-S shear zones have stronglycontrolled the extension of the main rupture segmentsand the aftershock distribution. The surface rupturesare located within the area of coseismic deformationresulting from DInSAR data; we propose that theyrepresent the localized response to the verticalground deformation of the area. Finally, we discussthe contribution of the pattern of the 1997 surfacebreaks to the characterization of the seismogenicsource.
    Type of Medium: Electronic Resource
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  • 2
    Publication Date: 2016-04-07
    Description: The article presents the results of the quantitative statistical analyses of the first world catalog of earthquake-rotated objects (EROs), presented in Part I of the study ( Cucci et al. , 2016 ). We searched for possible relations between the epicentral distance of EROs occurrence and a number of customary seismological observables, such as magnitude, intensity, focal mechanism, etc. The reliability of results is quantitatively checked by means of some suitable statistical tests. We found strong evidence of a clear log–linear dependence of the epicentral distance, to which an ERO can be observed, on the magnitude M w of the source event. We note that the probability of observing EROs near the epicentral area ( D 〈10 km) inversely decreases with the earthquake magnitude and that, for large earthquakes ( M w 8+), this probability remains significant (around 30%) beyond 100 km from the epicenter. Unexpectedly, we did not find significant relations between EROs occurrence and epicentral intensity, possibly because of high dispersion of intensity values. The data analyzed in the present study identifies intensity 6 as the lowest intensity for rotation occurrence; this is different from the main macroseismic scales, which indicate the EROs as a diagnostic of larger intensity degrees. This outcome could suggest the need for revision and for updating the diagnostics indicated in the intensity scales. As for the focal mechanisms of the seismic events, we found higher probabilities of observing rotations beyond 10 km distance from the epicenter of a thrust-faulting earthquake than for a normal-faulting earthquake. This probability reverses beyond 50 km distance, especially for high-magnitude seismic events. Our results indicate interesting insights to potential end users of the EROs catalog in the fields of historical seismology and earthquake engineering.
    Print ISSN: 0037-1106
    Electronic ISSN: 1943-3573
    Topics: Geosciences , Physics
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  • 3
    Publication Date: 2016-04-07
    Description: We present the first world catalog of earthquake-rotated objects (EROs). The catalog is composed of 2053 EROs originating during 184 earthquakes that occurred between 1349 and 2014. The catalog is organized into two tables that contain information about the source earthquakes and about the observed EROs, respectively. EROs are observed to occur following earthquakes in the M w  4.0–8.3 range at localities marked by intensities in the interval I=3.5 (Medvedev–Sponhauer–Karnik [MSK] scale) to I=11 (modified Mercalli intensity [MMI] scale) and at epicentral distances as far as 445 km. We also present some qualitative analyses of the basic details of the catalog with respect to the parameters of the two data tables. These, along with the most complete quantitative analyses of the catalog presented in Part II of the study ( Lombardi et al. , 2016 ), provide interesting clues to address possible relations between EROs occurrence and a number of customary seismological observables, such as magnitude, intensity, epicentral distance, and fault orientation. Finally, we suggest that the utilization of the present catalog will contribute to a better understanding of the mechanism that induces the EROs occurrence and ultimately to provide important insights into the applications for earthquake engineering. Online Material: Table of parameters and information associated with the 2053 observations of earthquake-rotated objects.
    Print ISSN: 0037-1106
    Electronic ISSN: 1943-3573
    Topics: Geosciences , Physics
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  • 4
    Publication Date: 2015-01-29
    Description: The M  ~ 7 1915 Fucino (Central Italy) earthquake represents one of the most destructive seismic events ever occurred in the Italian Peninsula. Several seismogenic faults have been proposed in the past decades as the source of the earthquake by means of different approaches and techniques that lead to a variety of speculations about the source mechanism and the fault location, often contrasting with one another. The 1915 earthquake produced a remarkable data set of 73 coseismic hydrological changes in the near and intermediate field that consist in variation of the flow of streams and springs, liquefaction, rise of water temperature and turbidity. In this paper, we study the coseismic water level changes induced by the 1915 earthquake in the near field to provide convincing clues on the geometry of the earthquake causative fault. We model the coseismic strain field induced by seventeen individual faults proposed through different approaches, and compare its pattern with the distribution of streamflow changes. We find: (i) clues on the most probable geometry of the earthquake causative fault. Best fits between modelled deformation and observed data are displayed by sources (derived by geological or seismological data) that share several distinctive features, as they are ~135°-striking, SW-dipping, 25–30-km-long normal faults located along the eastern side of the Fucino basin. These data point to the Serrone Fault and the Parasano Fault as the most likely causative structures and support the hypothesis that the coseismic ruptures observed in the field represented primary surface faulting. On the contrary, our calculations show that the Pescina Fault and the Ventrino Fault are secondary faults from the perspective of the hydrological response. Finally, one of the best scoring potential sources (from geological data) is a multifaulting system that considers the presence, in the central-western part of the basin, of fault splays synthetic and antithetic to the main seismogenic structures; therefore, we infer for these splays a possible active involvement in a 1915-like seismogenic process; (ii) evidence against a number of seismogenic structures that were previously associated with the earthquake. In particular, the plots of coseismic strain induced by sources uniquely derived by macroseismic or geodetic data prove to be inconsistent with the polarities of the hydrological signatures. Also, sources mainly characterized by reverse faulting and/or by right-lateral strike-slip component are discarded and (iii) as a final remark, we maintain that the study of the hydrological signatures of earthquake strain can offer an alternative tool in the investigation of the historical seismicity, to estimate the focal mechanism of major earthquakes capable of giving rise to a consistent data set of hydrological data.
    Keywords: Seismology
    Print ISSN: 0956-540X
    Electronic ISSN: 1365-246X
    Topics: Geosciences
    Published by Oxford University Press on behalf of The Deutsche Geophysikalische Gesellschaft (DGG) and the Royal Astronomical Society (RAS).
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  • 5
    Publication Date: 2014-05-04
    Print ISSN: 0895-0695
    Electronic ISSN: 1938-2057
    Topics: Geosciences
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  • 6
    Publication Date: 2012-11-08
    Print ISSN: 0895-0695
    Electronic ISSN: 1938-2057
    Topics: Geosciences
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  • 7
    Publication Date: 2016-04-15
    Description: The article presents the results of the quantitative statistical analyses of the first world catalog of earthquake-rotated objects (EROs), presented in Part I of the study ( Cucci et al. , 2016 ). We searched for possible relations between the epicentral distance of EROs occurrence and a number of customary seismological observables, such as magnitude, intensity, focal mechanism, etc. The reliability of results is quantitatively checked by means of some suitable statistical tests. We found strong evidence of a clear log–linear dependence of the epicentral distance, to which an ERO can be observed, on the magnitude M w of the source event. We note that the probability of observing EROs near the epicentral area ( D 〈10 km) inversely decreases with the earthquake magnitude and that, for large earthquakes ( M w 8+), this probability remains significant (around 30%) beyond 100 km from the epicenter. Unexpectedly, we did not find significant relations between EROs occurrence and epicentral intensity, possibly because of high dispersion of intensity values. The data analyzed in the present study identifies intensity 6 as the lowest intensity for rotation occurrence; this is different from the main macroseismic scales, which indicate the EROs as a diagnostic of larger intensity degrees. This outcome could suggest the need for revision and for updating the diagnostics indicated in the intensity scales. As for the focal mechanisms of the seismic events, we found higher probabilities of observing rotations beyond 10 km distance from the epicenter of a thrust-faulting earthquake than for a normal-faulting earthquake. This probability reverses beyond 50 km distance, especially for high-magnitude seismic events. Our results indicate interesting insights to potential end users of the EROs catalog in the fields of historical seismology and earthquake engineering.
    Print ISSN: 0037-1106
    Electronic ISSN: 1943-3573
    Topics: Geosciences , Physics
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  • 8
    Publication Date: 2016-04-15
    Description: We present the first world catalog of earthquake-rotated objects (EROs). The catalog is composed of 2053 EROs originating during 184 earthquakes that occurred between 1349 and 2014. The catalog is organized into two tables that contain information about the source earthquakes and about the observed EROs, respectively. EROs are observed to occur following earthquakes in the M w  4.0–8.3 range at localities marked by intensities in the interval I=3.5 (Medvedev–Sponhauer–Karnik [MSK] scale) to I=11 (modified Mercalli intensity [MMI] scale) and at epicentral distances as far as 445 km. We also present some qualitative analyses of the basic details of the catalog with respect to the parameters of the two data tables. These, along with the most complete quantitative analyses of the catalog presented in Part II of the study ( Lombardi et al. , 2016 ), provide interesting clues to address possible relations between EROs occurrence and a number of customary seismological observables, such as magnitude, intensity, epicentral distance, and fault orientation. Finally, we suggest that the utilization of the present catalog will contribute to a better understanding of the mechanism that induces the EROs occurrence and ultimately to provide important insights into the applications for earthquake engineering. Online Material: Table of parameters and information associated with the 2053 observations of earthquake-rotated objects.
    Print ISSN: 0037-1106
    Electronic ISSN: 1943-3573
    Topics: Geosciences , Physics
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  • 9
    Publication Date: 2013-10-25
    Print ISSN: 0895-0695
    Electronic ISSN: 1938-2057
    Topics: Geosciences
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  • 10
    Publication Date: 2016-12-29
    Description: Though the Calabrian arc is the most seismic area of the Italian peninsula, the overwhelming majority of M 〉6.5 earthquakes have occurred during the last four centuries. Conversely, the Italian seismic catalog exhibits an almost total absence of earthquakes—even moderate-magnitude earthquakes—between the eleventh and sixteenth centuries. The reason for this anomalous distribution of seismicity can be partially accounted for by the lack of historical sources caused by a paucity of local archives and by the enduring isolation of local administrations. We focused our research on moderate-magnitude earthquakes of central-northern Calabria between the sixteenth and eighteenth centuries and performed systematic research in many repositories, including in the Archivio Segreto Vaticano, in the state Archives of Naples, Catanzaro, Cosenza, and Potenza, and in several historic libraries. We found 15 previously unknown earthquakes for which we provide the level of shaking and the indication of the epicentral area for the first time. Also, we could definitively categorize one further event as a landslide rather than an earthquake. Finally, we found new evidence and information about four seismic events already known in the seismological literature; in particular, we provide a new intensity map and an increased magnitude ( M  6.0) of the 14 July 1767 earthquake. Besides the new data on the earthquakes, we provide general clues and hints for searching useful documents to study earthquakes in the historical context of the sixteenth–eighteenth centuries.
    Print ISSN: 0895-0695
    Electronic ISSN: 1938-2057
    Topics: Geosciences
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