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FABIO REALE

Curriculum and Research

REALE FABIO

FABIO REALE

 (PHYS-05/A)

Fisica e Chimica - Emilio Segrè

Contacts

+3909123891743

fabio.reale@unipa.it

Download the curriculum in pdf file

Subjects

Academic Year Subject identification code Subject name ECTS Course of study
2024/2025 01501 ASTRONOMIA 6 SCIENZE FISICHE
2024/2025 22451 CLOUD AND HIGH PERFORMANCE COMPUTING 6 DATA, ALGORITHMS, AND MACHINE INTELLIGENCE
2024/2025 22419 SOLAR PHYSICS (MODULO) 3 FISICA
2024/2025 22425 SPACE WEATHER 6 FISICA

Publications

Date Title Type Record
2024 Coronal energy release by MHD avalanches II. EUV line emission from a multi-threaded coronal loop. Articolo in rivista Go to
2023 Asymmetric Twisting of Coronal Loops Articolo in rivista Go to
2023 Two-dimensional MHD modelling of switchbacks from jetlets in the slow solar wind Articolo in rivista Go to
2023 Coronal Heating Rate in the Slow Solar Wind Articolo in rivista Go to
2023 Coronal energy release by MHD avalanches Articolo in rivista Go to
2022 Linking Small-scale Solar Wind Properties with Large-scale Coronal Source Regions through Joint Parker Solar Probe-Metis/Solar Orbiter Observations Articolo in rivista Go to
2022 X-ray flares of the young planet host Ds Tucanae A Articolo in rivista Go to
2022 Connecting Solar Orbiter remote-sensing observations and Parker Solar Probe in situ measurements with a numerical MHD reconstruction of the Parker spiral Articolo in rivista Go to
2022 Probing the Physics of the Solar Atmosphere with the Multi-slit Solar Explorer (MUSE). I. Coronal Heating Articolo in rivista Go to
2021 Exploring the Solar Wind from Its Source on the Corona into the Inner Heliosphere during the First Solar Orbiter–Parker Solar Probe Quadrature Articolo in rivista Go to
2021 Tracing the ICME plasma with a MHD simulation Articolo in rivista Go to
2021 Slow-Mode Magnetoacoustic Waves in Coronal Loops Articolo in rivista Go to
2021 Quasi-Periodic Pulsations in Solar and Stellar Flares: A Review of Underpinning Physical Mechanisms and Their Predicted Observational Signatures Articolo in rivista Go to
2021 The first coronal mass ejection observed in both visible-light and UV HI Ly-α channels of the Metis coronagraph on board Solar Orbiter Articolo in rivista Go to
2021 Reconstruction of the Parker spiral with the Reverse in situ data and MHD APproach - RIMAP Articolo in rivista Go to
2021 Acoustic Wave Properties in Footpoints of Coronal Loops in 3D MHD Simulations Articolo in rivista Go to
2021 First light observations of the solar wind in the outer corona with the Metis coronagraph Articolo in rivista Go to
2021 The Heating of the Solar Corona Capitolo o Saggio Go to
2020 On the coronal temperature in solar microflares Articolo in rivista Go to
2020 Reconnection nanojets in the solar corona Articolo in rivista Go to
2019 Statistical Signatures of Nanoflare Activity. I. Monte Carlo Simulations and Parameter-space Exploration Articolo in rivista Go to
2019 Collisionless shock heating of heavy ions in SN 1987A Articolo in rivista Go to
2019 Deep X-ray view of the Class I YSO Elias 29 with XMM-Newton and NuSTAR Articolo in rivista Go to
2019 New view of the corona of classical T Tauri stars: Effects of flaring activity in circumstellar disks Articolo in rivista Go to
2019 Simultaneous Kepler/K2 and XMM-Newton observations of superflares in the Pleiades Articolo in rivista Go to
2019 Impulsive Coronal Heating from Large-scale Magnetic Rearrangements: From IRIS to SDO/AIA Articolo in rivista Go to
2019 A stellar flare-coronal mass ejection event revealed by X-ray plasma motions Articolo in rivista Go to
2019 Mass Accretion Impacts in Classical T Tauri Stars: A Multi-disciplinary Approach Contributo in atti di convegno pubblicato in volume Go to
2019 Large-amplitude Quasiperiodic Pulsations as Evidence of Impulsive Heating in Hot Transient Loop Systems Detected in the EUV with SDO/AIA Articolo in rivista Go to
2019 Simultaneous Kepler/K2 and XMM-Newton observations of superflares in the Pleiades Articolo in rivista Go to
2018 Guided flows in coronal magnetic flux tubes Articolo in rivista Go to
2018 Flaring activity on the disk of Classical T Tauri Stars: effects on disk stability Contributo in atti di convegno pubblicato in volume Go to
2018 Investigating the Response of Loop Plasma to Nanoflare Heating Using RADYN Simulations Articolo in rivista Go to
2018 X-Ray Flare Oscillations Track Plasma Sloshing along Star-disk Magnetic Tubes in the Orion Star-forming Region Articolo in rivista Go to
2017 Magnetic shuffling of coronal downdrafts Articolo in rivista Go to
2017 Spectroscopy of Very Hot Plasma in Non-flaring Parts of a Solar Limb Active Region: Spatial and Temporal Properties Articolo in rivista Go to
2017 The early B-type star Rho Ophiuchi A is an X-ray lighthouse Articolo in rivista Go to
2016 Modeling the shock-cloud interaction in SN 1006: Unveiling the origin of nonthermal X-ray and γ-ray emission Articolo in rivista Go to
2016 Impacts of fragmented accretion streams onto classical T Tauri stars: UV and X-ray emission lines Articolo in rivista Go to
2016 Bright Hot Impacts by Erupted Fragments Falling Back on the Sun: Magnetic Channelling Articolo in rivista Go to
2016 PLASMA SLOSHING IN PULSE-HEATED SOLAR AND STELLAR CORONAL LOOPS Articolo in rivista Go to
2016 3D MHD MODELING OF TWISTED CORONAL LOOPS Articolo in rivista Go to
2016 EUV FLICKERING OF SOLAR CORONAL LOOPS: A NEW DIAGNOSTIC OF CORONAL HEATING Articolo in rivista Go to
2016 Star-disk interaction in classical T Tauri stars revealed using wavelet analysis Articolo in rivista Go to
2016 X-RAYING THE DARK SIDE OF VENUS-SCATTER FROM VENUS' MAGNETOTAIL? Articolo in rivista Go to
2016 TIME-RESOLVED EMISSION FROM BRIGHT HOT PIXELS OF AN ACTIVE REGION OBSERVED IN THE EUV BAND WITH SDO/AIA AND MULTI-STRANDED LOOP MODELING Articolo in rivista Go to
2016 UV And X-Ray Emission from Impacts of Fragmented Accretion Streams on Classical T Tauri Stars Poster pubblicato in volume Go to
2016 Three X-ray flares near primary eclipse of the RS CVn binary XY UMa Articolo in rivista Go to
2015 ADAHELI+: exploring the fast, dynamic Sun in the x-ray, optical, and near-infrared Articolo in rivista Go to
2015 Using the transit of Venus to probe the upper planetary atmosphere Articolo in rivista Go to
2014 3D YSO accretion shock simulations: a study of the magnetic, chromospheric and stochastic flow effects Proceedings Go to
2014 Coronal Loops: Observations and Modeling of Confined Plasma Articolo in rivista Go to
2014 Probing the effects of hadronic acceleration at the SN 1006 shock front Contributo in atti di convegno pubblicato in rivista Go to
2014 MHD modelling of coronal loops: injection of high-speed chromospheric flows Articolo in rivista Go to
2014 MHD modeling of coronal loops: the transition region throat Articolo in rivista Go to
2014 X-rays from accretion shocks in classical T Tauri stars: 2D MHD modeling and the role of local absorption Proceedings Go to
2014 Thermal structure of a hot non-flaring corona from Hinode/EIS Articolo in rivista Go to
2014 3D numerical modeling of YSO accretion shocks Articolo in rivista Go to
2014 Bright hot impacts by erupted fragments falling back on the sun: Uv redshifts in stellar accretion Articolo in rivista Go to
2014 Evidence of nonthermal particles in coronal loops heated impulsively by nanoflares Articolo in rivista Go to
2014 Role of local absorption on the X-ray emission from MHD accretion shocks in classical T Tauri stars Articolo in rivista Go to
2013 Hydrodynamic modelling of ejecta shrapnel in the Vela supernova remnant Articolo in rivista Go to
2013 YSO accretion shocks: magnetic, chromospheric or stochastic flow effects can suppress fluctuations of X-ray emission Articolo in rivista Go to
2013 SphinX: The Solar Photometer in X-Rays Articolo in rivista Go to
2013 Bright Hot Impacts by Erupted Fragments Falling Back on the Sun: A Template for Stellar Accretion Articolo in rivista Go to
2013 XIPE: the X-ray imaging polarimetry explorer Articolo in rivista Go to
2013 Radiative accretion shocks along nonuniform stellar magnetic fields in classical T Tauri stars Articolo in rivista Go to
2013 PROMINENCE PLASMA DIAGNOSTICS THROUGH EXTREME-ULTRAVIOLET ABSORPTION Articolo in rivista Go to
2012 4th Hinode Science Meeting: Unsolved Problems and Recent Insights Curatela Go to
2012 Plasma Diagnostics and Magnetic Complexity of a Post-Flare Active Region with Hinode/XRT: Spatial and Temporal Evolution Proceedings Go to
2012 Monte Carlo Markov chain DEM reconstruction of isothermal plasmas Articolo in rivista Go to
2012 Hinode/EIS Spectroscopic Validation of Very Hot Plasma Imaged with the Solar Dynamics Observatory in Non-flaring Active Region Cores Articolo in rivista Go to
2012 SphinX Measurements of the 2009 Solar Minimum X-Ray Emission Articolo in rivista Go to
2012 Nanoflare Evidence from Analysis of the X-Ray Variability of an Active Region Observed with Hinode/XRT Proceedings Go to
2012 X-raying hadronic acceleration at the SN 1006 shock front Proceedings Go to
2012 Temperature Diagnostics of a Solar Active Region Using a Single-Filter Observation of Hinode/XRT Proceedings Go to
2012 Hot Plasma Detected in Active Regions by HINODE/XRT and SDO/AIA Proceedings Go to
2012 XMM-Newton evidence of shocked ISM in SN 1006: indications of hadronic acceleration Articolo in rivista Go to
2012 Chandra study of the eclipsing M dwarf binary, YY Gem Articolo in rivista Go to
2012 The Mouse that Roared: A SuperFlare from the dMe Flare Star EV Lac Detected by Swift and Konus-Wind Proceedings Go to
2012 The role of radiative losses in the late evolution of pulse-heated coronal loops/strands Articolo in rivista Go to
2012 Coronal structure and dynamics Proceedings Go to
2012 Dynamic Temperature Structure of the Corona Proceedings Go to
2012 X-ray emitting hot plasma in solar active regions observed by the SphinX spectrometer Articolo in rivista Go to
2012 Post-flare Ultraviolet Light Curves Explained with Thermal Instability of Loop Plasma Articolo in rivista Go to
2011 Solar Dynamics Observatory Discovers Thin High Temperature Strands in Coronal Active Regions Articolo in rivista Go to
2011 Multiwavelength diagnostics of accretion in an X-ray selected sample of CTTSs Articolo in rivista Go to
2011 Mass accretion to young stars triggered by flaring activity in circumstellar discs Articolo in rivista Go to
2011 Temperature Distribution of a Non-flaring Active Region from Simultaneous Hinode XRT and EIS Observations Articolo in rivista Go to
2011 SphinX soft X-ray spectrophotometer: Science objectives, design and performance Articolo in rivista Go to
2011 Widespread Nanoflare Variability Detected with Hinode/X-Ray Telescope in a Solar Active Region Articolo in rivista Go to
2010 Large Scale Properties of Coronal Heating along the Solar Cycle Proceedings Go to
2010 On the observability of T Tauri accretion shocks in the X-ray band Articolo in rivista Go to
2010 A Detailed Study of the Rise Phase of a Long Duration X-Ray Flare in the Young Star TWA 11B Articolo in rivista Go to
2010 Post-flare evolution of AR 10923 with Hinode/XRT Articolo in rivista Go to
2010 On the importance of background subtraction in the analysis of coronal loops observed with TRACE Abstract in rivista Go to
2010 An iterative method in a probabilistic approach to the spectral inverse problem - Differential emission measure from line spectra and broadband data Articolo in rivista Go to
2010 The Mouse That Roared: A Superflare from the dMe Flare Star EV Lac Detected by Swift and Konus-Wind Articolo in rivista Go to
2010 Observability and diagnostics in the X-ray band of shock-cloud interactions in supernova remnants Articolo in rivista Go to
2010 The EM(T) of stellar coronae Proceedings Go to
2010 Coronal Fuzziness Modeled with Pulse-heated Multi-stranded Loop Systems Articolo in rivista Go to
2010 Spatial identification of the overionized plasma in W49B Articolo in rivista Go to
2010 X-ray emitting MHD accretion shocks in classical T Tauri stars. Case for moderate to high plasma-β values Articolo in rivista Go to
2010 Coronal Loops: Observations and Modeling of Confined Plasma Articolo in rivista Go to
2010 X-ray Flares of EV Lac: Statistics, Spectra, and Diagnostics Articolo in rivista Go to
2009 Hydrodynamic Modeling of Accretion Shock on CTTSs Proceedings Go to
2009 Flaring Activity in Accretion Flows of Young Stellar Objects Proceedings Go to
2009 Effects of Flaring Activity on Dynamics of Accretion Disks in YSOs Proceedings Go to
2009 Multi-wavelength diagnostics of accretion in an X-ray selected sample of CTTSs Proceedings Go to
2009 MHD modeling of supernova remnants expanding through inhomogeneous interstellar medium Proceedings Go to
2009 Evidence of Widespread Hot Plasma in a Nonflaring Coronal Active Region from Hinode/X-Ray Telescope Articolo in rivista Go to
2009 Modeling accretion shocks on CTTSs and their X-ray emission Proceedings Go to
2009 Accretion shock on CTTSs and its X-ray emission Proceedings Go to
2009 Modeling SNR shock waves expanding through the magnetized inhomogeneous interstellar medium Articolo in rivista Go to
2009 Modeling the long duration rise phase of a flare detected on the M star TWA 11 B Proceedings Go to
2009 The Sun as a benchmark of flaring activity in stellar coronae Proceedings Go to
2009 Comparison of Hinode/XRT and RHESSI Detection of Hot Plasma in the Non-Flaring Solar Corona Articolo in rivista Go to
2008 Fine Thermal Structure of a Flare Observed with Hinode/XRT Proceedings Go to
2008 Fe Kα and Hydrodynamic Loop Model Diagnostics for a Large Flare on II Pegasi Articolo in rivista Go to
2008 Calibration of the SphinX experiment at the XACT facility in Palermo Proceedings Go to
2008 New constraints on chemical abundances of the shocked plasma in the supernova remnant IC443 Proceedings Go to
2008 A coronal explosion on the flare star CN Leonis Articolo in rivista Go to
2008 SphinX: A fast solar Photometer in X-rays Articolo in rivista Go to
2008 X-ray emission from dense plasma in classical T Tauri stars: hydrodynamic modeling of the accretion shock Articolo in rivista Go to
2008 High Performance Computing on the COMETA Grid Infrastructure Proceedings Go to
2008 Geometry Diagnostics of a Stellar Flare from Fluorescent X-Rays Articolo in rivista Go to
2008 MHD Modeling of Accretion Processes in Young Stars with the PLUTO Code Proceedings Go to
2008 Numerical Simulations and Diagnostics in Astrophysics: A few Magnetohydrodynamics Examples Proceedings Go to
2008 The flaring and quiescent components of the solar corona Articolo in rivista Go to
2008 Nonequilibrium of Ionization and the Detection of Hot Plasma in Nanoflare-heated Coronal Loops Articolo in rivista Go to
2008 Hydrodynamic modeling of ejecta shrapnels in the Vela SNR Proceedings Go to
2008 The Importance of Magnetic-Field-Oriented Thermal Conduction in the Interaction of SNR Shocks with Interstellar Clouds Articolo in rivista Go to
2008 Modeling magnetohydrodynamics and non-equilibrium SoHO/UVCS line emission of CME shocks Articolo in rivista Go to
2008 Hinode/XRT Diagnostics of Loop Thermal Structure Proceedings Go to
2007 Fine Thermal Structure of a Coronal Active Region Articolo in rivista Go to
2007 Modeling Magnetohydrodynamics And Non Equilibrium SoHO/UVCS Line Emission Of Cme Shocks Proceedings Go to
2007 Methods of Analyzing Temperatures in Post-Flare Loops using the XRT on Hinode Proceedings Go to
2007 X-ray flares on the UV Ceti-type star CC Eridani: a ``peculiar'' time-evolution of spectral parameters Articolo in rivista Go to
2007 X-ray flares in Orion low-mass stars Articolo in rivista Go to
2007 MHD evolution of a fragment of a CME core in the outer solar corona Articolo in rivista Go to
2007 Detailed Diagnostics of an X-Ray Flare in the Single Giant HR 9024 Articolo in rivista Go to
2007 On the origin of asymmetries in bilateral supernova remnants Articolo in rivista Go to
2007 Diagnostics of stellar flares from X-ray observations: from the decay to the rise phase Articolo in rivista Go to
2007 Magnetic activity and the solar corona: first results from the Hinode satellite Proceedings Go to
2006 Diagnostics of Coronal Loops from Multi-Band Observations Proceedings Go to
2006 X-raying the interstellar medium: the study of SNR shells at the OAPa Proceedings Go to
2006 Shock-cloud interaction in the Vela SNR. II. Hydrodynamic model Articolo in rivista Go to
2006 Crushing of interstellar gas clouds in supernova remnants. II. X-ray emission Articolo in rivista Go to
2006 Effect of the Magnetic Field on the Propagation of Coronal Mass Ejections Proceedings Go to
2006 Stationary and Flaring Heating Effect on the Coronal Emission Measure Proceedings Go to
2006 Flare diagnostics from loop modeling of a stellar flare observed with XMM-Newton Articolo in rivista Go to
2006 XMM-Newton Observations of the Supernova Remnant IC 443. I. Soft X-Ray Emission from Shocked Interstellar Medium Articolo in rivista Go to
2006 X-ray flare modeling in the single giant HR 9024 Proceedings Go to
2006 Hydrodynamic interaction of SNR shocks with thermally conducting, radiative clouds Proceedings Go to
2006 The Corona of the Sun as a Star Proceedings Go to
2006 Analysis of a multi-wavelength time-resolved observation of a coronal loop Articolo in rivista Go to
2006 X-ray and optical bursts and flares in YSOs: results from a 5-day XMM-Newton monitoring campaign of L1551 Articolo in rivista Go to
2005 Hydrodynamic simulations of the shock-cloud interaction in the Vela supernova remnant Capitolo o Saggio Go to
2005 Multi-phase interstellar clouds in the Vela SNR resolved with XMM-Newton Articolo in rivista Go to
2005 Sub-Structuring Dynamics and Heating in Dense Coronal Structures Proceedings Go to
2005 XMM-Newton observations of the young open cluster Blanco 1. II. X-ray time variability and flares. Articolo in rivista Go to
2005 Crushing of interstellar gas clouds in supernova remnants. I. The role of thermal conduction and radiative losses Articolo in rivista Go to
2005 X-ray observations of the young open cluster Blanco 1. The XMM-Newton view Proceedings Go to
2005 Modeling a coronal loop heated by magnetohydrodynamic turbulence nanoflares Articolo in rivista Go to
2005 Mhd-Modeling of the Propagation of a Coronal Mass Ejection Proceedings Go to
2005 Bright X-Ray Flares in Orion Young Stars from COUP: Evidence for Star-Disk Magnetic Fields? Articolo in rivista Go to
2005 Emission Measure Distribution in Loops Impulsively Heated at the Footpoints Articolo in rivista Go to
2005 3-Dimensional hydrodynamic interaction of a supernova remnant shock with an isolated cloud Proceedings Go to
2005 Shock-cloud interaction in the Vela SNR observed with XMM-Newton Articolo in rivista Go to
2004 Shock-cloud interaction in the Vela SNR: the XMM-Newton view Proceedings Go to
2004 An X-rays study of the shock-cloud interaction in the Vela SNR Proceedings Go to
2004 Are Coronae of Late-Type Stars Made of Solar-like Structures? The X-Ray Surface Flux versus Hardness Ratio Diagram and the Pressure-Temperature Correlation Articolo in rivista Go to
2004 The coronae of bright late-type stars observed with EPIC and RGS Proceedings Go to
2004 Modeling an X-ray flare on Proxima Centauri: Evidence of two flaring loop components and of two heating mechanisms at work Articolo in rivista Go to
2004 Using AMR to Simulate the 3-D Hydrodynamic Interaction of Supernova Shocks with Interstellar Gas Clouds Proceedings Go to
2004 Flares from small to large: X-ray spectroscopy of Proxima Centauri with XMM-Newton Articolo in rivista Go to
2004 Crushing of interstellar gas clouds in supernova remnants: The role of thermal conduction and radiative losses Proceedings Go to
2004 A large X-ray flare from the Herbig Ae star V892 Tau Articolo in rivista Go to
2004 Shock-cloud interaction in the Vela SNR: the XMM-Newton view Proceedings Go to
2004 The Sun as an X-ray star: Active region evolution, rotational modulation, and implications for stellar X-ray variability Articolo in rivista Go to
2003 Viewing the sun as an x-ray star Proceedings Go to
2002 Temperature and density structure of hot and cool loops derived from the analysis of trace data Proceedings Go to
2002 CALOS: an experiment to study the solar corona with an array of NTD Ge microcalorimeters Proceedings Go to
2001 The OAPA/DPSFA: Solar physics, instrumental expertise, and the XACT facility Proceedings Go to