42 citations · 249 across the 13 of their papers we have counts for
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ASR: Archival Solar flaRes catalogue
M. Berretti, S. Mestici, L. Giovannelli +4
Solar flares result from the rapid conversion of stored magnetic energy within the Sun's corona. These energy releases are associated with coronal magnetic loops, which are rooted…
The dynamics of small-scale magnetic fields modulated by the solar cycle
M. Stangalini, G. Verth, V. Fedun +9
In addition to sunspots, which represent the most easily visualized manifestation of solar magnetism, cutting-edge observations of the solar atmosphere have uncovered a plethora of…
Occurrence and persistence of magnetic elements in the quiet Sun
F. Giannattasio, F. Berrilli, G. Consolini +3
Turbulent convection efficiently transports energy up to the solar photosphere, but its multi-scale nature and dynamic properties are still not fully understood. Several works in t…
Polarised kink waves in magnetic elements: evidence for chromospheric helical waves
Marco Stangalini, Fabio Giannattasio, Robertus Erdélyi +6
In recent years, new high spatial resolution observations of the Sun's atmosphere have revealed the presence of a plethora of small-scale magnetic elements down to the resolution l…
Plasma flows and magnetic field interplay during the formation of a pore
I. Ermolli, A. Cristaldi, F. Giorgi +5
We studied the formation of a pore in AR NOAA 11462. We analysed data obtained with the IBIS at the DST on April 17, 2012, consisting of full Stokes measurements of the Fe I 617.3…
N-body model of magnetic flux tubes reconnecting in the solar atmosphere
Luca Giovannelli, Francesco Berrilli, Dario Del Moro +7
The investigation of dynamics of the small scale magnetic field on the Sun photosphere is necessary to understand the physical processes occurring in the higher layers of solar atm…
Non-linear propagation of kink waves to the solar chromosphere
M. Stangalini, F. Giannattasio, S. Jafarzadeh
Small-scale magnetic field concentrations (magnetic elements) in the quiet Sun are believed to contribute to the energy budget of the upper layers of the Sun's atmosphere, as they…
Super-diffusion versus competitive advection: a simulation
D. Del Moro, F. Giannattasio, F. Berrilli +3
Magnetic element tracking is often used to study the transport and diffusion of the magnetic field on the solar photosphere. From the analysis of the displacement spectrum of these…
Diffusion of magnetic elements in a supergranular cell
F. Giannattasio, M. Stangalini, F. Berrilli +2
Small scale magnetic fields (magnetic elements) are ubiquitous in the solar photosphere. Their interaction can provide energy to the upper atmospheric layers, and contribute to hea…
Diffusion of solar magnetic elements up to supergranular spatial and temporal scales
F. Giannattasio, D. Del Moro, F. Berrilli +3
The study of spatial and temporal scales on which small magnetic structures (magnetic elements) are organized in the quiet Sun may be approached by determining how they are transpo…
On the asymmetry of velocity oscillation amplitude in bipolar active regions
F. Giannattasio, M. Stangalini, D. Del Moro +1
The velocity field in the lower solar atmosphere undergoes strong interactions with magnetic fields. Many authors have pointed out that power is reduced by a factor between two and…
High cadence spectropolarimetry of moving magnetic features observed around a pore
S. Criscuoli, D. Del Moro, F. Giannattasio +5
Moving magnetic features (MMFs) are small-size magnetic elements that are seen to stream out from sunspots, generally during their decay phase. Several observational results presen…
Three-minute wave enhancement in the solar photosphere
M. Stangalini, F. Giannattasio, D. Del Moro +1
It is a well-known result that the power of five-minute oscillations is progressively reduced by magnetic fields in the solar photosphere. Many authors have pointed out that this f…