5 citations · 5 across the 1 of their papers we have counts for
6 papers
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…
Oblique tearing mode instability: guide field and Hall effect
Chen Shi, Marco Velli, Fulvia Pucci +2
The tearing mode instability is one important mechanism that may explain the triggering of fast magnetic reconnection in astrophysical plasmas such as the solar corona and the Eart…
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…
Dynamic evolution of current sheets, ideal tearing, plasmoid formation and generalized fractal reconnection scaling relations
Alkendra Singh, Fulvia Pucci, Anna Tenerani +3
Magnetic reconnection may be the fundamental process allowing energy stored in magnetic fields to be released abruptly, solar flares and coronal mass ejection (CME) being archetypa…
Properties of turbulence in the reconnection exhaust: numerical simulations compared with observations
F. Pucci, S. Servidio, L. Sorriso-Valvo +6
The properties of the turbulence which develops in the outflows of magnetic reconnection have been investigated using self-consistent plasma simulations, in three dimensions. As co…
The "ideal" tearing mode: theory and resistive MHD simulations
L. Del Zanna, S. Landi, E. Papini +2
Classical MHD reconnection theories, both the stationary Sweet-Parker model and the tearing instability, are known to provide rates which are too slow to explain the observations.…