Eleonora Amato
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Research Subjects
Eleonora Amato has a total of 19 co-authors. Here are the top co-authors by number of shared publications:
- Ciro Del Negro
Sezione Osservatorio Etneo, Istituto Nazionale di Geofisica e Vulcanologia (INGV), 95125 Catania, Italy
16 shared publications - Claudia Corradino
Istituto Nazionale di Geofisica e Vulcanologia, Sezione di Catania, Osservatorio Etneo, Piazza Roma 2, 95125 Catania, Italy
13 shared publications - Federica Torrisi
Istituto Nazionale di Geofisica e Vulcanologia, Sezione di Catania, Osservatorio Etneo, 95125 Catania, Italy
12 shared publications Vito Zago
Istituto Nazionale di Geofisica e Vulcanologia, Sezione Osservatorio Etneo, Catania, Italy
5 shared publications- Vito Zago
Sezione Osservatorio Etneo, Istituto Nazionale di Geofisica e Vulcanologia (INGV), 95125 Catania, Italy
4 shared publications Simona Cariello
3 shared publications
Latest Publications
- Open Access
AI-Based Super-Resolution Approaches to Reconstruct Temperature Fields of Climatic Data Using Deep Neural Networks
High-fidelity climate analysis is heavily constrained both by the computational costs of high-resolution dynamical simulations and by the general scarcity of fine-scale observational data for model evaluation. To address these limitations, in this work we propose a deep learning framework for spatial climate downscaling using an AI-based super-resolution (SR) approach. We develop Deep Neural Network architectures designed to upscale 2 m surface temperature fields, bridging the gap between gridded global reanalysis data at lower scale (1.0°) and higher scale (0.25°). We developed three DNN models, specifically ResNet, RNN, and ConvRNN, trained and validated on ECMWF ERA5 data from the early years of the current millennium (i.e., of at 00:00) and evaluated over various periods, including 1992, a historical period influenced by the 1991 Mount Pinatubo eruption (a large volcanic eruption which is known to have had impacts on the climate due to the massive stratospheric injections of sulfur dioxide). The framework is tested also on the Berkeley Earth global observational dataset and on outputs from a MPI-ESM1-2-LR historical global climate simulation and compared with traditional interpolation methods, to verify the models generalization capability. The models reached high levels of accuracy, with errors lower than 0.5 K and a similarity index higher than 0.97, successfully capturing the spatio-temporal dynamics of temperature fields. Overall, the novelty of this work is in three main aspects: the implementation of DNN capable to capture the spatio-temporal dynamics and not only the static frame-by-frame processes, the combination of conventional pixel-based error metrics with morphological validation frameworks based on isoline pattern and gradient orientation comparison, and the introduction of optimized training strategies (i.e., early stopping), to improve learning mechanisms and balance computational costs.Open AccessAI-Based Super-Resolution Approaches to Reconstruct Temperature Fields of Climatic Data Using Deep Neural Networks
High-fidelity climate analysis is heavily constrained both by the computational costs of high-resolution dynamical simulations and by the general scarcity of fine-scale observational data for model evaluation. To address these limitations, in this work we propose a deep learning framework for spatial climate downscaling using an AI-based super-resolution (SR) approach. We develop Deep Neural Network architectures designed to upscale 2 m surface temperature fields, bridging the gap between gridded global reanalysis data at lower scale (1.0°) and higher scale (0.25°). We developed three DNN models, specifically ResNet, RNN, and ConvRNN, trained and validated on ECMWF ERA5 data from the early years of the current millennium (i.e., of at 00:00) and evaluated over various periods, including 1992, a historical period influenced by the 1991 Mount Pinatubo eruption (a large volcanic eruption which is known to have had impacts on the climate due to the massive stratospheric injections of sulfur dioxide). The framework is tested also on the Berkeley Earth global observational dataset and on outputs from a MPI-ESM1-2-LR historical global climate simulation and compared with traditional interpolation methods, to verify the models generalization capability. The models reached high levels of accuracy, with errors lower than 0.5 K and a similarity index higher than 0.97, successfully capturing the spatio-temporal dynamics of temperature fields. Overall, the novelty of this work is in three main aspects: the implementation of DNN capable to capture the spatio-temporal dynamics and not only the static frame-by-frame processes, the combination of conventional pixel-based error metrics with morphological validation frameworks based on isoline pattern and gradient orientation comparison, and the introduction of optimized training strategies (i.e., early stopping), to improve learning mechanisms and balance computational costs. - Open Access
- 13 October 2026
- Published by MDPI AG in Remote Sensing
- Vol. 18 (20) , 3510
Advanced AI-Based Techniques for Empirical Chronological Mapping of Lava Flows Using Multispectral Satellite Imagery: A Case Study of Mount Etna
Effusive volcanic eruptions pose significant hazards to populated areas, making the accurate dating of lava flows essential for reconstructing eruptive histories and assessing volcanic risk. Traditional dating techniques, such as radiometric, paleomagnetic and lichenometric methods, are highly reliable but require direct sampling, complex analytical procedures, and substantial financial resources. Satellite remote sensing provides a non-invasive and spatially extensive approach that can complement conventional methods in the regional investigation of exposed volcanic surfaces. This study presents a two-stage hybrid classification–regression framework for empirical age estimation and chronological mapping of historical lava surfaces on Mount Etna, spanning the 17th to the 21st centuries. In the first stage, a Random Forest Classifier distinguishes background, pre-1600 lava surfaces, and post-1600 historical lava surfaces, thereby defining the spatial applicability domain of the chronological model. In the second stage, a Random Forest Regressor estimates age only for pixels classified as post-1600 lava by integrating ten Sentinel-2 surface-reflectance bands, elevation derived from the Digital Elevation Model (DEM), and a binary north-flank spatial indicator. On the balanced pixel-level test dataset, the RFR achieved an of 0.549, a Mean Absolute Error of 66.2 years, and a Root Mean Squared Error of 89.0 years. Using the median prediction for each test eruption, the corresponding eruption-level values were , MAE years, and RMSE years. Prediction errors were larger for the oldest evaluated surfaces, indicating reduced empirical discrimination near the lower boundary of the calibrated chronological domain. This pattern may reflect calibration-boundary effects, sparse chronological coverage, eruption-specific variability, and possible convergence of surface spectral properties. Comparison with an RBF-SVR showed comparable but metric-dependent performance, without establishing the overall superiority of either regression architecture. Permutation analysis indicated that most predictive information within this dataset was associated with the Sentinel-2 spectral component, particularly the Red Edge bands. The proposed method should therefore be interpreted as a complementary fast empirical lava age-estimation and regional screening framework for exposed historical lava surfaces, rather than as a substitute for radiometric, paleomagnetic, or field-based dating.- 13 October 2026
- Published by MDPI AG in Remote Sensing
- Vol. 18 (20) , 3510
Open AccessAdvanced AI-Based Techniques for Empirical Chronological Mapping of Lava Flows Using Multispectral Satellite Imagery: A Case Study of Mount Etna
Effusive volcanic eruptions pose significant hazards to populated areas, making the accurate dating of lava flows essential for reconstructing eruptive histories and assessing volcanic risk. Traditional dating techniques, such as radiometric, paleomagnetic and lichenometric methods, are highly reliable but require direct sampling, complex analytical procedures, and substantial financial resources. Satellite remote sensing provides a non-invasive and spatially extensive approach that can complement conventional methods in the regional investigation of exposed volcanic surfaces. This study presents a two-stage hybrid classification–regression framework for empirical age estimation and chronological mapping of historical lava surfaces on Mount Etna, spanning the 17th to the 21st centuries. In the first stage, a Random Forest Classifier distinguishes background, pre-1600 lava surfaces, and post-1600 historical lava surfaces, thereby defining the spatial applicability domain of the chronological model. In the second stage, a Random Forest Regressor estimates age only for pixels classified as post-1600 lava by integrating ten Sentinel-2 surface-reflectance bands, elevation derived from the Digital Elevation Model (DEM), and a binary north-flank spatial indicator. On the balanced pixel-level test dataset, the RFR achieved an of 0.549, a Mean Absolute Error of 66.2 years, and a Root Mean Squared Error of 89.0 years. Using the median prediction for each test eruption, the corresponding eruption-level values were , MAE years, and RMSE years. Prediction errors were larger for the oldest evaluated surfaces, indicating reduced empirical discrimination near the lower boundary of the calibrated chronological domain. This pattern may reflect calibration-boundary effects, sparse chronological coverage, eruption-specific variability, and possible convergence of surface spectral properties. Comparison with an RBF-SVR showed comparable but metric-dependent performance, without establishing the overall superiority of either regression architecture. Permutation analysis indicated that most predictive information within this dataset was associated with the Sentinel-2 spectral component, particularly the Red Edge bands. The proposed method should therefore be interpreted as a complementary fast empirical lava age-estimation and regional screening framework for exposed historical lava surfaces, rather than as a substitute for radiometric, paleomagnetic, or field-based dating. - Open Access
- 3 April 2026
- Published by Elsevier in Computers & Fluids
- Vol. 313
A lagrangian AI-based CFD emulator with reconstruction of Hydrodynamic forces components
- 3 April 2026
- Published by Elsevier in Computers & Fluids
- Vol. 313
Open AccessA lagrangian AI-based CFD emulator with reconstruction of Hydrodynamic forces components
- Open Access
- 13 March 2026
- Published by Copernicus GmbH
Advanced computing technologies to enhance modeling of the climatic impacts of large explosive eruptions
The Earth’s climate system is highly complex and responds to several forcing mechanisms, both natural and anthropogenic, with significant short- and long-term societal impacts. Among natural forcings, large explosive volcanic eruptions represent the dominant driver of abrupt cooling episodes over the past two millennia. However, the limited number of well-documented events and the substantial uncertainties in eruption source parameters, initial conditions, and aerosol forcing make the quantitative assessment of volcano–climate interactions particularly challenging. Addressing these limitations requires the integration of large and heterogeneous datasets, from satellite observations and in situ measurements to historical and paleoclimate archives, within modeling tools capable of capturing the nonlinear dynamics of the climate system. Advanced computing technologies, such as Artificial Intelligence (AI), High-Performance Computing (HPC), and emerging Quantum Computing (QC), offer new opportunities to overcome these constraints. AI and hybrid Machine Learning–physics approaches can emulate computationally expensive model components, improve the representation of aerosol–radiation processes, and accelerate sensitivity analyses, while HPC and QC can reduce the cost of large ensemble simulations and discover hidden patterns. Here, we highlight how these methodologies can enhance the study of volcano-climate interactions, improving model performance, enabling a more efficient exploration of uncertainties, and refining predictions of the climatic impacts of major explosive eruptions.
- 13 March 2026
- Published by Copernicus GmbH
Open AccessAdvanced computing technologies to enhance modeling of the climatic impacts of large explosive eruptions
The Earth’s climate system is highly complex and responds to several forcing mechanisms, both natural and anthropogenic, with significant short- and long-term societal impacts. Among natural forcings, large explosive volcanic eruptions represent the dominant driver of abrupt cooling episodes over the past two millennia. However, the limited number of well-documented events and the substantial uncertainties in eruption source parameters, initial conditions, and aerosol forcing make the quantitative assessment of volcano–climate interactions particularly challenging. Addressing these limitations requires the integration of large and heterogeneous datasets, from satellite observations and in situ measurements to historical and paleoclimate archives, within modeling tools capable of capturing the nonlinear dynamics of the climate system. Advanced computing technologies, such as Artificial Intelligence (AI), High-Performance Computing (HPC), and emerging Quantum Computing (QC), offer new opportunities to overcome these constraints. AI and hybrid Machine Learning–physics approaches can emulate computationally expensive model components, improve the representation of aerosol–radiation processes, and accelerate sensitivity analyses, while HPC and QC can reduce the cost of large ensemble simulations and discover hidden patterns. Here, we highlight how these methodologies can enhance the study of volcano-climate interactions, improving model performance, enabling a more efficient exploration of uncertainties, and refining predictions of the climatic impacts of major explosive eruptions.
- Open Access
- 3 February 2026
- Published by Instituto Nazionale di Geofisica e Vulcanologia, INGV in Annals of Geophysics
- Vol. 69 (1) , V107
Simulations of Complex Visco-Thermal Fluids with an AI-based CFD Emulator
Physical phenomena evolve in space and time following governing laws with a high level of complexity and mathematical models can help to make accurate predictions of their behavior, describing complex fluids with a good balance between accuracy and computational costs. We have long used detailed Computational Fluid Dynamics (CFD) models to simulate complex dynamics with high accuracy, but these simulations typically entail high computational costs, resulting in long execution times and the use of expensive computational resources. To overcome these limitations, we have recently integrated CFD with Artificial Intelligence (AI), in the so-called Emulators, to expand the scope of fluid modeling, improving its performance. Here, we present an AI-based CFD emulator for Smoothed Particle Hydrodynamics (SPH) simulations, which uses an Artificial Neural Network (ANN) to enhance simulations of complex fluids with viscous and thermal components. We show the model capability to reproduce the spatio-temporal evolution of natural visco-thermal fluids. In addition, we demonstrate the emulator capacity to generalize its applicability to problems not encountered during the training phase. We also conduct a detailed error evaluation, showing that the minimal observed discrepancies do not compromise model accuracy and robustness, especially given the theoretical and computational advantages. These key points open this emulator to practical applications for natural fluids, e.g., oil, honey, or geophysical fluids such as lava, enhancing fluidmodeling performance and extending functionalities. The innovation of this method improves studies in the field of numerical simulations, for example in its use as a digital Twin of a physical phenomenon, for the study of the dynamics of the system without the need of large costs for field analysis or laboratory experiments.
- 3 February 2026
- Published by Instituto Nazionale di Geofisica e Vulcanologia, INGV in Annals of Geophysics
- Vol. 69 (1) , V107
Open AccessSimulations of Complex Visco-Thermal Fluids with an AI-based CFD Emulator
Physical phenomena evolve in space and time following governing laws with a high level of complexity and mathematical models can help to make accurate predictions of their behavior, describing complex fluids with a good balance between accuracy and computational costs. We have long used detailed Computational Fluid Dynamics (CFD) models to simulate complex dynamics with high accuracy, but these simulations typically entail high computational costs, resulting in long execution times and the use of expensive computational resources. To overcome these limitations, we have recently integrated CFD with Artificial Intelligence (AI), in the so-called Emulators, to expand the scope of fluid modeling, improving its performance. Here, we present an AI-based CFD emulator for Smoothed Particle Hydrodynamics (SPH) simulations, which uses an Artificial Neural Network (ANN) to enhance simulations of complex fluids with viscous and thermal components. We show the model capability to reproduce the spatio-temporal evolution of natural visco-thermal fluids. In addition, we demonstrate the emulator capacity to generalize its applicability to problems not encountered during the training phase. We also conduct a detailed error evaluation, showing that the minimal observed discrepancies do not compromise model accuracy and robustness, especially given the theoretical and computational advantages. These key points open this emulator to practical applications for natural fluids, e.g., oil, honey, or geophysical fluids such as lava, enhancing fluidmodeling performance and extending functionalities. The innovation of this method improves studies in the field of numerical simulations, for example in its use as a digital Twin of a physical phenomenon, for the study of the dynamics of the system without the need of large costs for field analysis or laboratory experiments.
- Open Access
- 15 May 2025
- Published by Copernicus GmbH
Combining numerical CFD models and AI to enhance lava flow simulations
Lava flows are complex, non-Newtonian fluids with visco-thermal dependencies that can overcome barriers, form tunnels, and significantly impact surrounding areas. Understanding and predicting these flows are critical for quantifying volcanic hazards. Computational Fluid Dynamics (CFD) models are indispensable tools for simulating lava dynamics, but they often entail high computational costs, limiting their real-time applicability. To address these challenges, we propose an AI-enhanced CFD emulator for lava flows, designed to improve modeling efficiency while preserving accuracy. Our approach integrates AI with CFD to capture the visco-thermal properties of lava and its intricate dynamics, including phase transitions, particle solidification, and the influence of air on thermal behavior. The emulator has been validated through simulations of diverse physical scenarios, demonstrating its capability to generalize across varying conditions. Additionally, we conducted a sensitivity analysis, exploring the influence of key parameters, such as effusion rate, on lava flow evolution and eruption styles. By incorporating satellite-derived estimates, we provide insights into eruptive behaviors while minimizing the risks of field observations. Our results showcase the potential of combining AI, numerical models, and remote sensing to enhance traditional volcanic monitoring approaches. This hybrid methodology enables faithful, near real-time simulations of lava flows, offering valuable tools for hazard assessment and risk mitigation.
- 15 May 2025
- Published by Copernicus GmbH
Open AccessCombining numerical CFD models and AI to enhance lava flow simulations
Lava flows are complex, non-Newtonian fluids with visco-thermal dependencies that can overcome barriers, form tunnels, and significantly impact surrounding areas. Understanding and predicting these flows are critical for quantifying volcanic hazards. Computational Fluid Dynamics (CFD) models are indispensable tools for simulating lava dynamics, but they often entail high computational costs, limiting their real-time applicability. To address these challenges, we propose an AI-enhanced CFD emulator for lava flows, designed to improve modeling efficiency while preserving accuracy. Our approach integrates AI with CFD to capture the visco-thermal properties of lava and its intricate dynamics, including phase transitions, particle solidification, and the influence of air on thermal behavior. The emulator has been validated through simulations of diverse physical scenarios, demonstrating its capability to generalize across varying conditions. Additionally, we conducted a sensitivity analysis, exploring the influence of key parameters, such as effusion rate, on lava flow evolution and eruption styles. By incorporating satellite-derived estimates, we provide insights into eruptive behaviors while minimizing the risks of field observations. Our results showcase the potential of combining AI, numerical models, and remote sensing to enhance traditional volcanic monitoring approaches. This hybrid methodology enables faithful, near real-time simulations of lava flows, offering valuable tools for hazard assessment and risk mitigation.
- Open Access
- 20 January 2025
- Published by Copernicus GmbH
Generalizability of AI-based Emulators for CFD Lagrangian methods
The combination of Computational Fluid Dynamics (CFD) and Artificial Intelligence (AI) enables to expand the scope of fluid modeling and improve simulation performance. Eulerian methods have already been extensively integrated with AI, providing high-fidelity and reliable results (e.g., weather prediction); the application of AI to Lagrangian methods remains less consolidated. Smoothed Particle Hydrodynamics (SPH) is a Lagrangian mesh-less CFD numerical method with well-established advantages for the simulation of highly dynamic free-surface complex fluids. However, reliable SPH simulations require long execution times and large computational resources. This downside can be resolved using emulators, which can reproduce the dynamics of a physical system, speeding-up the simulations. In detail, an emulator is a model in which AI algorithms join or replace the equation-based mathematical representation of physics. Thus, the emulator learns from CFD simulations the behavior of the CFD reference model and reproduces it to solve fluid dynamics problems in shorter times. For the emulator to be trusted, it is important to assess the ability to generalize and correctly predict the behavior of the fluid in conditions that have not been presented during training phase. Here, we present the generalizability of an AI-based emulator for SPH, utilizing an Artificial Neural Network (ANN) to estimate the hydrodynamic forces between SPH particles. We demonstrate the capability of the emulator to reproduce particle interaction quantities, as opposed to their specific spatial configuration. Therefore, when a different problem is treated, as long as the variables values are in a range with physics meaning presented during training, the emulator will be capable to produce physically meaningful results. We discuss the salient points of designing this emulator, such as the choice of the AI model, i.e., the ANN, and the choice of the features. We show applications to different test cases, highlighting the emulator ability to generalize for problems with varying levels of complexity, and for changes in the model resolution.
- 20 January 2025
- Published by Copernicus GmbH
Open AccessGeneralizability of AI-based Emulators for CFD Lagrangian methods
The combination of Computational Fluid Dynamics (CFD) and Artificial Intelligence (AI) enables to expand the scope of fluid modeling and improve simulation performance. Eulerian methods have already been extensively integrated with AI, providing high-fidelity and reliable results (e.g., weather prediction); the application of AI to Lagrangian methods remains less consolidated. Smoothed Particle Hydrodynamics (SPH) is a Lagrangian mesh-less CFD numerical method with well-established advantages for the simulation of highly dynamic free-surface complex fluids. However, reliable SPH simulations require long execution times and large computational resources. This downside can be resolved using emulators, which can reproduce the dynamics of a physical system, speeding-up the simulations. In detail, an emulator is a model in which AI algorithms join or replace the equation-based mathematical representation of physics. Thus, the emulator learns from CFD simulations the behavior of the CFD reference model and reproduces it to solve fluid dynamics problems in shorter times. For the emulator to be trusted, it is important to assess the ability to generalize and correctly predict the behavior of the fluid in conditions that have not been presented during training phase. Here, we present the generalizability of an AI-based emulator for SPH, utilizing an Artificial Neural Network (ANN) to estimate the hydrodynamic forces between SPH particles. We demonstrate the capability of the emulator to reproduce particle interaction quantities, as opposed to their specific spatial configuration. Therefore, when a different problem is treated, as long as the variables values are in a range with physics meaning presented during training, the emulator will be capable to produce physically meaningful results. We discuss the salient points of designing this emulator, such as the choice of the AI model, i.e., the ANN, and the choice of the features. We show applications to different test cases, highlighting the emulator ability to generalize for problems with varying levels of complexity, and for changes in the model resolution.
- Open Access
- 25 July 2023
- Published by MDPI AG in Remote Sensing
- Vol. 15 (15) , 3718
A Deep Convolutional Neural Network for Detecting Volcanic Thermal Anomalies from Satellite Images
The latest generation of high-spatial-resolution satellites produces measurements of high-temperature volcanic features at global scale, which are valuable to monitor volcanic activity. Recent advances in technology and increased computational resources have resulted in an extraordinary amount of monitoring data, which can no longer be so readily examined. Here, we present an automatic detection algorithm based on a deep convolutional neural network (CNN) that uses infrared satellite data to automatically determine the presence of volcanic thermal activity. We exploit the potentiality of the transfer learning technique to retrain a pre-trained SqueezeNet CNN to a new domain. We fine-tune the weights of the network over a new dataset opportunely created with images related to thermal anomalies of different active volcanoes around the world. Furthermore, an ensemble approach is employed to enhance accuracy and robustness when compared to using individual models. We chose a balanced training dataset with two classes, one containing volcanic thermal anomalies (erupting volcanoes) and the other containing no thermal anomalies (non-erupting volcanoes), to differentiate between volcanic scenes with eruptive and non-eruptive activity. We used satellite images acquired in the infrared bands by ESA Sentinel-2 Multispectral Instrument (MSI) and NASA & USGS Landsat 8 Operational Land Imager and Thermal InfraRed Sensor (OLI/TIRS). This deep learning approach makes the model capable of identifying the appearance of a volcanic thermal anomaly in the images belonging to the volcanic domain with an overall accuracy of 98.3%, recognizing the scene with active flows and erupting vents (i.e., eruptive activity) and the volcanoes at rest. This model is generalizable, and has the capability to analyze every image captured by these satellites over volcanoes around the world.
- 25 July 2023
- Published by MDPI AG in Remote Sensing
- Vol. 15 (15) , 3718
Open AccessA Deep Convolutional Neural Network for Detecting Volcanic Thermal Anomalies from Satellite Images
The latest generation of high-spatial-resolution satellites produces measurements of high-temperature volcanic features at global scale, which are valuable to monitor volcanic activity. Recent advances in technology and increased computational resources have resulted in an extraordinary amount of monitoring data, which can no longer be so readily examined. Here, we present an automatic detection algorithm based on a deep convolutional neural network (CNN) that uses infrared satellite data to automatically determine the presence of volcanic thermal activity. We exploit the potentiality of the transfer learning technique to retrain a pre-trained SqueezeNet CNN to a new domain. We fine-tune the weights of the network over a new dataset opportunely created with images related to thermal anomalies of different active volcanoes around the world. Furthermore, an ensemble approach is employed to enhance accuracy and robustness when compared to using individual models. We chose a balanced training dataset with two classes, one containing volcanic thermal anomalies (erupting volcanoes) and the other containing no thermal anomalies (non-erupting volcanoes), to differentiate between volcanic scenes with eruptive and non-eruptive activity. We used satellite images acquired in the infrared bands by ESA Sentinel-2 Multispectral Instrument (MSI) and NASA & USGS Landsat 8 Operational Land Imager and Thermal InfraRed Sensor (OLI/TIRS). This deep learning approach makes the model capable of identifying the appearance of a volcanic thermal anomaly in the images belonging to the volcanic domain with an overall accuracy of 98.3%, recognizing the scene with active flows and erupting vents (i.e., eruptive activity) and the volcanoes at rest. This model is generalizable, and has the capability to analyze every image captured by these satellites over volcanoes around the world.
- Open Access
- 15 May 2023
- Published by Copernicus GmbH
On Artificial Intelligence-based emulators of physical models to forecast the evolution of lava flows
Timely forecasting of the evolution of lava flows is one of the key elements for assessing volcanic hazards. Lava flows are among the main hazardous phenomena during an effusive eruption, due to the possibility to reach urban areas and cause damage to infrastructure. Physical-mathematical models can be used to estimate the dynamics of a fluid or the fluid-solid interactions, in particular for the case of lava flows. However, high fidelity models require long execution times and large computational resources. Recently, artificial intelligence (AI) has been adopted to emulate physics-based models and deliver similar results, speeding up the simulations. We will discuss the possibility to use AI-based approaches to emulate highly complex numerical models used to simulate the spatio-temporal evolution of lava flows. Analyzing and treating the formal mathematical aspects of the models under analysis, we will verify and validate the models using test cases associated with the main features of lavas, discussing the accuracy and the performance offered by the two approaches.
- 15 May 2023
- Published by Copernicus GmbH
Open AccessOn Artificial Intelligence-based emulators of physical models to forecast the evolution of lava flows
Timely forecasting of the evolution of lava flows is one of the key elements for assessing volcanic hazards. Lava flows are among the main hazardous phenomena during an effusive eruption, due to the possibility to reach urban areas and cause damage to infrastructure. Physical-mathematical models can be used to estimate the dynamics of a fluid or the fluid-solid interactions, in particular for the case of lava flows. However, high fidelity models require long execution times and large computational resources. Recently, artificial intelligence (AI) has been adopted to emulate physics-based models and deliver similar results, speeding up the simulations. We will discuss the possibility to use AI-based approaches to emulate highly complex numerical models used to simulate the spatio-temporal evolution of lava flows. Analyzing and treating the formal mathematical aspects of the models under analysis, we will verify and validate the models using test cases associated with the main features of lavas, discussing the accuracy and the performance offered by the two approaches.
- Open Access
- 26 February 2023
- Published by Copernicus GmbH
An Artificial Intelligence-based platform for volcanic hazard monitoring
Satellite remote sensing data are suitable to monitor global scale volcanic hazards in an efficient and timely manner. The development of monitoring systems which automatically collect and process satellite data is crucial during a volcanic crisis. The huge amount of multispectral satellite data available requires new approaches capable of processing them automatically and artificial intelligence (AI) addresses these needs. Machine learning, a type of AI in which computers learn from data, is gaining importance in volcanology. The combination of ML algorithms and satellite remote sensing in volcano monitoring has the potential of analyzing global data in near real-time for mapping and monitoring purposes. Here, an AI-based platform was developed to monitor in near real-time the volcanic activity from space. AI algorithms are used to retrieve information about the ongoing volcanic activity. Under this perspective, a key role is played by ML since it overcomes the issues related to hard coded/explicit rules by implicitly learning them from historical satellite data. Volcanic eruptions are then fully characterized in terms of their energy release, e.g. volcanic radiative power (VRP), effusive rate, quantification of the erupted products, i.e. volume, spatial extension, volcanic cloud composition. This task is achieved by combining a variety of freely available satellite datasets, i.e. infrared (IR) data with different spatial, temporal and spectral features. In particular, both a geostationary satellite sensor, i.e. SEVIRI (Spinning Enhanced Visible and InfraRed Imager, on board Meteosat satellites), and several mid-high spatial resolution polar satellite sensors, e.g. MODIS (Moderate Resolution Imaging Spectroradiometer, on board Terra and Aqua satellites), VIIRS (Visible Infrared Imaging Radiometer Suite, on board the Suomi-NPP and NOAA-20 satellites), SLSTR (Sea and Land Surface Temperature Radiometer, on board Sentinel-3A and Sentinel-3B satellites), MSI (MultiSpectral Instrument, on board Sentinel-2), are adopted. We demonstrate the potential of this web-based satellite-data-driven platform during the recent eruptive events on Stromboli and Etna.
- 26 February 2023
- Published by Copernicus GmbH
Open AccessAn Artificial Intelligence-based platform for volcanic hazard monitoring
Satellite remote sensing data are suitable to monitor global scale volcanic hazards in an efficient and timely manner. The development of monitoring systems which automatically collect and process satellite data is crucial during a volcanic crisis. The huge amount of multispectral satellite data available requires new approaches capable of processing them automatically and artificial intelligence (AI) addresses these needs. Machine learning, a type of AI in which computers learn from data, is gaining importance in volcanology. The combination of ML algorithms and satellite remote sensing in volcano monitoring has the potential of analyzing global data in near real-time for mapping and monitoring purposes. Here, an AI-based platform was developed to monitor in near real-time the volcanic activity from space. AI algorithms are used to retrieve information about the ongoing volcanic activity. Under this perspective, a key role is played by ML since it overcomes the issues related to hard coded/explicit rules by implicitly learning them from historical satellite data. Volcanic eruptions are then fully characterized in terms of their energy release, e.g. volcanic radiative power (VRP), effusive rate, quantification of the erupted products, i.e. volume, spatial extension, volcanic cloud composition. This task is achieved by combining a variety of freely available satellite datasets, i.e. infrared (IR) data with different spatial, temporal and spectral features. In particular, both a geostationary satellite sensor, i.e. SEVIRI (Spinning Enhanced Visible and InfraRed Imager, on board Meteosat satellites), and several mid-high spatial resolution polar satellite sensors, e.g. MODIS (Moderate Resolution Imaging Spectroradiometer, on board Terra and Aqua satellites), VIIRS (Visible Infrared Imaging Radiometer Suite, on board the Suomi-NPP and NOAA-20 satellites), SLSTR (Sea and Land Surface Temperature Radiometer, on board Sentinel-3A and Sentinel-3B satellites), MSI (MultiSpectral Instrument, on board Sentinel-2), are adopted. We demonstrate the potential of this web-based satellite-data-driven platform during the recent eruptive events on Stromboli and Etna.