60 citations · 325 across the 15 of their papers we have counts for
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Applications of Fast Magnetic Reconnection Models to the Atmospheres of the Sun and Protoplanetary Disks
Fulvia Pucci, Alkendra Singh, Uma Gorti +4
Partially-ionized plasmas consist of charged and neutral particles whose mutual collisions modify magnetic reconnection compared with the fully-ionized case. The collisions alter t…
Transition region from turbulent to dead zone in protoplanetary disks: local shearing box simulations
Fulvia Pucci, Kengo Tomida, James Stone +3
The dynamical evolution of protoplanetary disks is of key interest for building a comprehensive theory of planet formation and to explain the observational properties of these obje…
Tearing modes in partially ionized plasmas
Fulvia Pucci, K. Alkendra P. Singh, Anna Tenerani +1
In many astrophysical environments the plasma is only partially ionized, and therefore the interaction of charged and neutral particles may alter both the triggering of reconnectio…
Fast Magnetic Reconnection: "Ideal" Tearing and the Hall Effect
Fulvia Pucci, Marco Velli, Anna Tenerani
One of the main questions in magnetic reconnection is the origin of triggering behavior with on/off properties that accounts, once it is activated, for the fast magnetic energy con…
"Ideally" unstable current sheets and the triggering of fast magnetic reconnection
Anna Tenerani, Marco Velli, Fulvia Pucci +2
Magnetic reconnection is thought to be the dynamical mechanism underlying many explosive phenomena observed both in space and in the laboratory, though the question of how fast mag…
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…