New radio observations at cold fronts in galaxy clusters lead to the proposal that magnetic reconnection, rather than Fermi acceleration, re-accelerates particles at these contact discontinuities.
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2 Pith papers cite this work. Polarity classification is still indexing.
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2026 2verdicts
UNVERDICTED 2representative citing papers
In the fully plasmoid-mediated regime the reconnection rate becomes nearly independent of the magnetic Prandtl number.
citing papers explorer
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Magnetic Reconnection in Galaxy Clusters
New radio observations at cold fronts in galaxy clusters lead to the proposal that magnetic reconnection, rather than Fermi acceleration, re-accelerates particles at these contact discontinuities.
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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.