Tommaso Alberti

Dr. Tommaso Alberti

INAF-Istituto di Astrofisica e Planetologia Spaziali, via del Fosso del Cavaliere 100, 00133 Rome, Italy
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Research Focus & Metrics

Academic Career Length

13Years (2014-Present)

(Calculated once Scilit publication data is synced: current year − year of first publication + 1)

Representative Publications

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31 October 2017 in Solar Physics
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Journal Article
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Mirko PiersantiMirko Piersanti
Mirko Piersanti
Tommaso AlbertiTommaso Alberti
Tommaso Alberti
ABAlessandro Bemporad
Alessandro Bemporad
BFBerrilli Francesco
Berrilli Francesco
RBRoberto Bruno
Roberto Bruno
JLJános Lichtenberger
János Lichtenberger

1 November 2020 in Chaos: An Interdisciplinary Journal of Nonlinear Science
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Journal Article
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DFDavide Faranda
Davide Faranda
Tommaso AlbertiTommaso Alberti
Tommaso Alberti
COVID-19 has forced quarantine measures in several countries across the world. These measures have proven to be effective in significantly reducing the prevalence of the virus. To date, no effective treatment or vaccine is available. In the effort of preserving both public health and the economical and social textures, France and Italy governments have partially released lockdown measures. Here, we extrapolate the long-term behavior of the epidemic in both countries using a susceptible-exposed-infected-recovered model, where parameters are stochastically perturbed with a lognormal distribution to handle the uncertainty in the estimates of COVID-19 prevalence and to simulate the presence of super-spreaders. Our results suggest that uncertainties in both parameters and initial conditions rapidly propagate in the model and can result in different outcomes of the epidemic leading or not to a second wave of infections. Furthermore, the presence of super-spreaders adds instability to the dynamics, making the control of the epidemic more difficult. Using actual knowledge, asymptotic estimates of COVID-19 prevalence can fluctuate of the order of 10 × 10 6 units in both countries.

24 July 2024 in Weather and Climate Dynamics
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Journal Article
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DFDavide Faranda
Davide Faranda
GMGabriele Messori
Gabriele Messori
ECErika Coppola
Erika Coppola
Tommaso AlbertiTommaso Alberti
Tommaso Alberti
MVMathieu Vrac
Mathieu Vrac
RVRobert Vautard
Robert Vautard
Climate change is a global challenge with multiple far-reaching consequences, including the intensification and increased frequency of many extreme-weather events. In response to this pressing issue, we present ClimaMeter, a platform designed to assess and contextualize extreme-weather events relative to climate change. The platform offers near-real-time insights into the dynamics of extreme events, serving as a resource for researchers and policymakers while also being a science dissemination tool for the general public. ClimaMeter currently analyses heatwaves, cold spells, heavy precipitation, and windstorms. This paper elucidates the methodology, data sources, and analytical techniques on which ClimaMeter relies, providing a comprehensive overview of its scientific foundation. We further present two case studies: the late 2023 French heatwave and the July 2023 Storm Poly. We use two distinct datasets for each case study, namely Multi-Source Weather (MSWX) data, which serve as the reference for our rapid-attribution protocol, and the ERA5 dataset, widely regarded as the leading global climate reanalysis. These examples highlight both the strengths and limitations of ClimaMeter in expounding the link between climate change and the dynamics of extreme-weather events.

19 April 2017 in Journal of Geophysical Research: Space Physics
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Tommaso AlbertiTommaso Alberti
Tommaso Alberti
Giuseppe ConsoliniGiuseppe Consolini
Giuseppe Consolini
FLFabio Lepreti
Fabio Lepreti
MLMonica Laurenza
Monica Laurenza
AVA. Vecchio
A. Vecchio
Vincenzo CarboneVincenzo Carbone
Vincenzo Carbone

25 March 2019 in Entropy
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Journal Article
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Tommaso AlbertiTommaso Alberti
Tommaso Alberti
Giuseppe ConsoliniGiuseppe Consolini
Giuseppe Consolini
Vincenzo CarboneVincenzo Carbone
Vincenzo Carbone
EYEmiliya Yordanova
Emiliya Yordanova
MMMaria Federica Marcucci
Maria Federica Marcucci
PMPaola De Michelis
Paola De Michelis
Turbulence, intermittency, and self-organized structures in space plasmas can be investigated by using a multifractal formalism mostly based on the canonical structure function analysis with fixed constraints about stationarity, linearity, and scales. Here, the Empirical Mode Decomposition (EMD) method is firstly used to investigate timescale fluctuations of the solar wind magnetic field components; then, by exploiting the local properties of fluctuations, the structure function analysis is used to gain insights into the scaling properties of both inertial and kinetic/dissipative ranges. Results show that while the inertial range dynamics can be described in a multifractal framework, characterizing an unstable fixed point of the system, the kinetic/dissipative range dynamics is well described by using a monofractal approach, because it is a stable fixed point of the system, unless it has a higher degree of complexity and chaos.

1 June 2020 in Communications in Nonlinear Science and Numerical Simulation
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Journal Article
Closed access
Tommaso AlbertiTommaso Alberti
Tommaso Alberti
DFDavide Faranda
Davide Faranda