Francesca Bianco
Current Organizations / Institutes
The organizations/institutes from the scholar's latest article
Previous Organizations / Institutes
The organizations / institutes from the scholar's other articles in the past ten years
Research Subjects
Francesca Bianco has a total of 164 co-authors. Here are the top co-authors by number of shared publications:
- Edoardo Del Pezzo
Osservatorio Vesuviano, Naples, Italy
35 shared publications Edoardo Del Pezzo
Sezione Osservatorio Vesuviano
8 shared publications- Lucia Zaccarelli
INGV
8 shared publications - Gilberto Saccorotti
Istituto Nazionale di Geofisica e Vulcanologia, Pisa, Italy
6 shared publications - Jesus M. Ibanez
Department of Theoretical Physics and Cosmos University of Granada Granada Spain
6 shared publications - Luca De Siena
Dipartimento di Fisica e Astronomia “Augusto Righi”, Alma Mater Studiorum Università di Bologna, 40126 Bologna, Italy
6 shared publications
Latest Publications
- Open Access
- 1 January 2025
- Published by Seismological Society of America (SSA) in The Seismic Record
- Vol. 5 (1) , 1-10
The Energy Space Density (ESD) Distribution: A New Approach to Reveal the Degree of Fracturing of the Crust in the Etna Region (Italy)
The traditional method of representing the seismicity in a region involves plotting earthquakes of various magnitudes on a map. Energy release, however, offers a different perspective for understanding seismicity, especially in volcanic areas where earthquakes are abundant and occur in the form of swarms. In this study, we analyzed earthquakes with a moment magnitude (Mw) greater than 1.5 that occurred between 2006 and 2023, which were relocated using a 3D velocity model, to examine the distribution of energy space density (ESD) in the Etna region. The ESD maps reveal the fundamental patterns of seismicity, which generally align with the local structural features. The shallow crust above 10 km plays a crucial role in energy distribution, with the highest values found in the eastern and southwestern sectors, along well-known structures bordering the unstable sector of the volcano. At deeper levels (down to 20 km), high ESD values are observed in the western sector and are related to the dynamics of magma movement at these depths. The ESD pattern improves the clarity of rock fracture density visualization, offering a more detailed view of the areas with the highest fracture density. These regions may indicate where fluid is stored beneath the volcano.
- 1 January 2025
- Published by Seismological Society of America (SSA) in The Seismic Record
- Vol. 5 (1) , 1-10
Open AccessThe Energy Space Density (ESD) Distribution: A New Approach to Reveal the Degree of Fracturing of the Crust in the Etna Region (Italy)
The traditional method of representing the seismicity in a region involves plotting earthquakes of various magnitudes on a map. Energy release, however, offers a different perspective for understanding seismicity, especially in volcanic areas where earthquakes are abundant and occur in the form of swarms. In this study, we analyzed earthquakes with a moment magnitude (Mw) greater than 1.5 that occurred between 2006 and 2023, which were relocated using a 3D velocity model, to examine the distribution of energy space density (ESD) in the Etna region. The ESD maps reveal the fundamental patterns of seismicity, which generally align with the local structural features. The shallow crust above 10 km plays a crucial role in energy distribution, with the highest values found in the eastern and southwestern sectors, along well-known structures bordering the unstable sector of the volcano. At deeper levels (down to 20 km), high ESD values are observed in the western sector and are related to the dynamics of magma movement at these depths. The ESD pattern improves the clarity of rock fracture density visualization, offering a more detailed view of the areas with the highest fracture density. These regions may indicate where fluid is stored beneath the volcano.
- Open Access
- 9 May 2024
- Published by Elsevier in Earth and Planetary Science Letters
- Vol. 637
Tracking transient changes in the plumbing system at Campi Flegrei Caldera
- 9 May 2024
- Published by Elsevier in Earth and Planetary Science Letters
- Vol. 637
Open AccessTracking transient changes in the plumbing system at Campi Flegrei Caldera
- Open Access
- 3 January 2024
- Published by Springer Nature in Pure and Applied Geophysics
- Vol. 181 (1) , 171-187
Depth and Spatial Variation of the Shear Wave Attenuation Parameters in the Shallow Crust and Lower Crust/Upper Mantle of Mt. Etna (Italy)
Seismic wave attenuation is a key feature of seismic wave propagation that provides constraints on the composition and physical state of the medium within the Earth. We separated intrinsic and scattering attenuation coefficients for the shallow crust and lower crust/upper mantle in the Mt. Etna area. For this purpose, the Multiple Lapse Time Window Analysis (MLTWA) was applied to two groups of earthquakes, well separated in depth. We also studied the spatial variation of the attenuation parameters by dividing the study area into four sectors around Etna. The results show an effective homogeneity of the propagation characteristics inside Etna and, in particular, some lateral variations and minor variations with depth. We observe that structural discontinuities and lithology control scattering losses at all frequencies, with higher scattering in the shallow crust. The intrinsic absorption shows no sensitivity to the presence of these main geological structures and is quite uniform for different depths. Furthermore, compared to the northern sector of the volcano, the southern one shows stronger scattering attenuation at low frequencies. This pattern correlates well with the high seismic activity along most of Etna’s active tectonic structures and ascending magmatic fluids that characterize this sector of the volcano. Although we only discuss the differences in the "average" scattering and inelastic properties of the investigated volumes, the results of this study are very informative about the characteristics of each region. Moreover, they suggest that a future study is necessary, providing a more detailed picture of the spatial distribution of seismic attenuation in the study area, through a 3D inversion of the attenuation parameters estimated along the single source-receiver paths.
- 3 January 2024
- Published by Springer Nature in Pure and Applied Geophysics
- Vol. 181 (1) , 171-187
Open AccessDepth and Spatial Variation of the Shear Wave Attenuation Parameters in the Shallow Crust and Lower Crust/Upper Mantle of Mt. Etna (Italy)
Seismic wave attenuation is a key feature of seismic wave propagation that provides constraints on the composition and physical state of the medium within the Earth. We separated intrinsic and scattering attenuation coefficients for the shallow crust and lower crust/upper mantle in the Mt. Etna area. For this purpose, the Multiple Lapse Time Window Analysis (MLTWA) was applied to two groups of earthquakes, well separated in depth. We also studied the spatial variation of the attenuation parameters by dividing the study area into four sectors around Etna. The results show an effective homogeneity of the propagation characteristics inside Etna and, in particular, some lateral variations and minor variations with depth. We observe that structural discontinuities and lithology control scattering losses at all frequencies, with higher scattering in the shallow crust. The intrinsic absorption shows no sensitivity to the presence of these main geological structures and is quite uniform for different depths. Furthermore, compared to the northern sector of the volcano, the southern one shows stronger scattering attenuation at low frequencies. This pattern correlates well with the high seismic activity along most of Etna’s active tectonic structures and ascending magmatic fluids that characterize this sector of the volcano. Although we only discuss the differences in the "average" scattering and inelastic properties of the investigated volumes, the results of this study are very informative about the characteristics of each region. Moreover, they suggest that a future study is necessary, providing a more detailed picture of the spatial distribution of seismic attenuation in the study area, through a 3D inversion of the attenuation parameters estimated along the single source-receiver paths.
- 1 January 2022
- Published by Springer Nature
- p. 55-94
Seismic and Gravity Structure of the Campi Flegrei Caldera, Italy
- 1 January 2022
- Published by Springer Nature
- p. 55-94
Seismic and Gravity Structure of the Campi Flegrei Caldera, Italy
- 1 January 2022
- Published by Springer Nature
- p. 219-237
The Permanent Monitoring System of the Campi Flegrei Caldera, Italy
- 1 January 2022
- Published by Springer Nature
- p. 219-237
The Permanent Monitoring System of the Campi Flegrei Caldera, Italy
- Open Access
- 2 August 2019
- Published by MDPI AG in Remote Sensing
- Vol. 11 (15) , 1813
Integration of Ground-Based Remote-Sensing and In Situ Multidisciplinary Monitoring Data to Analyze the Eruptive Activity of Stromboli Volcano in 2017–2018
After a period of mild eruptive activity, Stromboli showed between 2017 and 2018 a reawakening phase, with an increase in the eruptive activity starting in May 2017. The alert level of the volcano was raised from “green” (base) to “yellow” (attention) on 7 December 2017, and a small lava overflowed the crater rim on 15 December 2017. Between July 2017 and August 2018 the monitoring networks recorded nine major explosions, which are a serious hazard for Stromboli because they affect the summit area, crowded by tourists. We studied the 2017–2018 eruptive phase through the analysis of multidisciplinary data comprising thermal video-camera images, seismic, geodetic and geochemical data. We focused on the major explosion mechanism analyzing the well-recorded 1 December 2017 major explosion as a case study. We found that the 2017–2018 eruptive phase is consistent with a greater gas-rich magma supply in the shallow system. Furthermore, through the analysis of the case study major explosion, we identified precursory phases in the strainmeter and seismic data occurring 77 and 38 s before the explosive jet reached the eruptive vent, respectively. On the basis of these short-term precursors, we propose an automatic timely alarm system for major explosions at Stromboli volcano.
- 2 August 2019
- Published by MDPI AG in Remote Sensing
- Vol. 11 (15) , 1813
Open AccessIntegration of Ground-Based Remote-Sensing and In Situ Multidisciplinary Monitoring Data to Analyze the Eruptive Activity of Stromboli Volcano in 2017–2018
After a period of mild eruptive activity, Stromboli showed between 2017 and 2018 a reawakening phase, with an increase in the eruptive activity starting in May 2017. The alert level of the volcano was raised from “green” (base) to “yellow” (attention) on 7 December 2017, and a small lava overflowed the crater rim on 15 December 2017. Between July 2017 and August 2018 the monitoring networks recorded nine major explosions, which are a serious hazard for Stromboli because they affect the summit area, crowded by tourists. We studied the 2017–2018 eruptive phase through the analysis of multidisciplinary data comprising thermal video-camera images, seismic, geodetic and geochemical data. We focused on the major explosion mechanism analyzing the well-recorded 1 December 2017 major explosion as a case study. We found that the 2017–2018 eruptive phase is consistent with a greater gas-rich magma supply in the shallow system. Furthermore, through the analysis of the case study major explosion, we identified precursory phases in the strainmeter and seismic data occurring 77 and 38 s before the explosive jet reached the eruptive vent, respectively. On the basis of these short-term precursors, we propose an automatic timely alarm system for major explosions at Stromboli volcano.
- Open Access
- 5 July 2018
- Published by American Geophysical Union (AGU) in Geophysical Research Letters
- Vol. 45 (13) , 6428-6436
Ambient Seismic Noise Image of the Structurally Controlled Heat and Fluid Feeder Pathway at Campi Flegrei Caldera
Earthquakes at Campi Flegrei have been low magnitude and sparse since 1985, denying onshore monitoring observations of their usual source for structural constraint: seismic tomography. Here we used continuous seismic records from 2011–2013 to reconstruct period‐dependent Rayleigh wave group velocity maps of the volcano. The Neapolitan Yellow Tuff rim faults bound high‐velocity intracrater products of historical eruptions, which act as a barrier for deep fluid migration. The anomaly with lowest group velocity is aseismic and corresponds to the portion of a fluid storage zone that was fractured during the 1984 volcanic unrest under Pozzuoli town. Earthquake locations show that fluids migrate from this area toward the Solfatara and Pisciarelli fumaroles along shallower low‐velocity fractures. The aseismic anomaly is likely fed by a deep‐seated offshore magmatic source. Its spatial relation with regional dynamics and observations from historical unrests mark the area as the most likely feeder pathway for fluid and magmatic inputs from depth.
- 5 July 2018
- Published by American Geophysical Union (AGU) in Geophysical Research Letters
- Vol. 45 (13) , 6428-6436
Open AccessAmbient Seismic Noise Image of the Structurally Controlled Heat and Fluid Feeder Pathway at Campi Flegrei Caldera
Earthquakes at Campi Flegrei have been low magnitude and sparse since 1985, denying onshore monitoring observations of their usual source for structural constraint: seismic tomography. Here we used continuous seismic records from 2011–2013 to reconstruct period‐dependent Rayleigh wave group velocity maps of the volcano. The Neapolitan Yellow Tuff rim faults bound high‐velocity intracrater products of historical eruptions, which act as a barrier for deep fluid migration. The anomaly with lowest group velocity is aseismic and corresponds to the portion of a fluid storage zone that was fractured during the 1984 volcanic unrest under Pozzuoli town. Earthquake locations show that fluids migrate from this area toward the Solfatara and Pisciarelli fumaroles along shallower low‐velocity fractures. The aseismic anomaly is likely fed by a deep‐seated offshore magmatic source. Its spatial relation with regional dynamics and observations from historical unrests mark the area as the most likely feeder pathway for fluid and magmatic inputs from depth.
- Open Access
- 11 May 2018
- Published by MDPI AG in Geosciences
- Vol. 8 (5) , 175
Numerically Calculated 3D Space-Weighting Functions to Image Crustal Volcanic Structures Using Diffuse Coda Waves
Seismic coda measurements retrieve parameters linked to the physical characteristics of rock volumes illuminated by high frequency scattered waves. Space weighting functions (SWF) and kernels are different tools that model the spatial sensitivity of coda envelopes to scattering and absorption anomalies in these rock matrices, allowing coda-wave attenuation ( ) imaging. This note clarifies the difference between SWF and sensitivity kernels developed for coda wave imaging. It extends the SWF previously developed in 2D to the third dimension by using radiative transfer and the diffusion equation, based on the assumption that variations of depend solely on variations of the extinction length. When applied to active data (Deception Island, Antarctica), 3D SWF images strongly resemble 2D images, making this 3D extension redundant. On the other hand, diffusion does not efficiently model coda waveforms when using earthquake datasets spanning depths between 0 and 20 km, such as at Mount St. Helens volcano. In this setting, scattering attenuation and absorption suffer tradeoffs and cannot be separated by fitting a single seismogram energy envelope for SWF imaging. We propose that an approximate analytical 3D SWF, similar in shape to the common coda kernels used in literature, can still be used in a space weighted back-projection approach. While is not a physical parameter of the propagation medium, its spatially-dependent modeling allows improved reconstruction of crustal-scale tectonic and geological features. It is even more efficient as a velocity independent imaging tool for magma and fluid storage when applied to deep volcanism.- 11 May 2018
- Published by MDPI AG in Geosciences
- Vol. 8 (5) , 175
Open AccessNumerically Calculated 3D Space-Weighting Functions to Image Crustal Volcanic Structures Using Diffuse Coda Waves
Seismic coda measurements retrieve parameters linked to the physical characteristics of rock volumes illuminated by high frequency scattered waves. Space weighting functions (SWF) and kernels are different tools that model the spatial sensitivity of coda envelopes to scattering and absorption anomalies in these rock matrices, allowing coda-wave attenuation ( ) imaging. This note clarifies the difference between SWF and sensitivity kernels developed for coda wave imaging. It extends the SWF previously developed in 2D to the third dimension by using radiative transfer and the diffusion equation, based on the assumption that variations of depend solely on variations of the extinction length. When applied to active data (Deception Island, Antarctica), 3D SWF images strongly resemble 2D images, making this 3D extension redundant. On the other hand, diffusion does not efficiently model coda waveforms when using earthquake datasets spanning depths between 0 and 20 km, such as at Mount St. Helens volcano. In this setting, scattering attenuation and absorption suffer tradeoffs and cannot be separated by fitting a single seismogram energy envelope for SWF imaging. We propose that an approximate analytical 3D SWF, similar in shape to the common coda kernels used in literature, can still be used in a space weighted back-projection approach. While is not a physical parameter of the propagation medium, its spatially-dependent modeling allows improved reconstruction of crustal-scale tectonic and geological features. It is even more efficient as a velocity independent imaging tool for magma and fluid storage when applied to deep volcanism. - 2 March 2018
- Published by American Geophysical Union (AGU) in Geophysical Research Letters
- Vol. 45 (5) , 2193-2202
The 21 August 2017 Ischia (Italy) Earthquake Source Model Inferred From Seismological, GPS, and DInSAR Measurements
- 2 March 2018
- Published by American Geophysical Union (AGU) in Geophysical Research Letters
- Vol. 45 (5) , 2193-2202
The 21 August 2017 Ischia (Italy) Earthquake Source Model Inferred From Seismological, GPS, and DInSAR Measurements
- 15 March 2017
- Published by American Geophysical Union (AGU) in Geophysical Research Letters
- Vol. 44 (5) , 2237-2244
Noise‐based seismic monitoring of the Campi Flegrei caldera
The Campi Flegrei caldera is one of the highest risk volcanic fields worldwide, because of its eruptive history and the large population hosted within the caldera. It experiences bradiseismic crises: sudden uplift with low energetic seismic swarm occurrences. No seismicity is recorded out of these deformation rate changes. Therefore, a continuous seismic monitoring of the caldera is possible only by means of the ambient seismic noise. We apply a noise‐based seismic monitoring technique to the cross correlations of 5 year recordings at the mobile seismic network. The resulting relative velocity variations are compared to the temporal behavior of the geophysical and geochemical observations routinely sampled at Campi Flegrei. We discriminate between two kinds of crustal stress field variations acting at different timescales. They are related to a possible magmatic intrusion and to the gradual heating of the hydrothermal system, respectively. This study sets up the basis for future volcano monitoring strategies.
- 15 March 2017
- Published by American Geophysical Union (AGU) in Geophysical Research Letters
- Vol. 44 (5) , 2237-2244
Noise‐based seismic monitoring of the Campi Flegrei caldera
The Campi Flegrei caldera is one of the highest risk volcanic fields worldwide, because of its eruptive history and the large population hosted within the caldera. It experiences bradiseismic crises: sudden uplift with low energetic seismic swarm occurrences. No seismicity is recorded out of these deformation rate changes. Therefore, a continuous seismic monitoring of the caldera is possible only by means of the ambient seismic noise. We apply a noise‐based seismic monitoring technique to the cross correlations of 5 year recordings at the mobile seismic network. The resulting relative velocity variations are compared to the temporal behavior of the geophysical and geochemical observations routinely sampled at Campi Flegrei. We discriminate between two kinds of crustal stress field variations acting at different timescales. They are related to a possible magmatic intrusion and to the gradual heating of the hydrothermal system, respectively. This study sets up the basis for future volcano monitoring strategies.