The collisionless reconnection rate decreases with increasing system size when initial current sheet thickness scales proportionally, eliminating the apparent universal fast rate of ~0.1.
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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
3D MHD modeling reveals Y-points do not coincide with cusp tips in candle-flame flares and apparent downflow speeds underestimate Alfvén speeds by 2-10x due to projection effects.
citing papers explorer
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System Size Dependence of Collisionless Reconnection Rate
The collisionless reconnection rate decreases with increasing system size when initial current sheet thickness scales proportionally, eliminating the apparent universal fast rate of ~0.1.
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On the Nature of Candle-Flame-Shaped Solar Flares and Sub-Alfv\'enic Supra-Arcade Plasma Downflows
3D MHD modeling reveals Y-points do not coincide with cusp tips in candle-flame flares and apparent downflow speeds underestimate Alfvén speeds by 2-10x due to projection effects.