In the fully plasmoid-mediated regime the reconnection rate becomes nearly independent of the magnetic Prandtl number.
bound- ary shearing of an initially homogeneous magnetic field
2 Pith papers cite this work. Polarity classification is still indexing.
2
Pith papers citing it
years
2026 2verdicts
UNVERDICTED 2representative citing papers
3D rMHD simulations show coronal nanojets originate in cool dense plasma during reconnection, explaining their collimation and visibility across wavelengths.
citing papers explorer
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Magnetic Prandtl number dependence of plasmoid-mediated reconnection
In the fully plasmoid-mediated regime the reconnection rate becomes nearly independent of the magnetic Prandtl number.
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On the cool nature of coronal nanojets
3D rMHD simulations show coronal nanojets originate in cool dense plasma during reconnection, explaining their collimation and visibility across wavelengths.