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physics.plasm-ph2020
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…
physics.plasm-ph2019
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…