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Updated: Jun 5, 2026

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Published on: August 1, 2017
Fast magnetic reconnection in the plasmoid-dominated regime
D A Uzdensky1, N F Loureiro, A A Schekochihin
1Center for Integrated Plasma Studies, University of Colorado, Boulder, Colorado 80309, USA.
A new model explains magnetic reconnection using a chain of plasmoids. The reconnection rate is independent of the Lundquist number, with a probability of large plasmoids causing disruptions in space and fusion plasmas.
Area of Science:
- Plasma Physics
- Astrophysics
- Fusion Energy
Background:
- Magnetic reconnection is a fundamental process in plasma physics, crucial for phenomena like solar flares and sawtooth crashes in fusion devices.
- Understanding the dynamics of resistive magnetic reconnection, particularly the role of plasmoids, is essential for predicting and controlling these events.
Purpose of the Study:
- To propose a conceptual model for resistive magnetic reconnection based on a stochastic plasmoid chain.
- To investigate the dependence of the global reconnection rate on plasma parameters and the flux distribution within plasmoids.
- To identify conditions leading to the formation of large plasmoids and their potential impact on reconnection dynamics and observable events.
Main Methods:
- Development of a conceptual model for resistive magnetic reconnection.
- Analytical investigation of the global reconnection rate and plasmoid flux distribution.
- Probabilistic analysis of the emergence of large plasmoids.
- Derivation of a criterion for the transition between resistive magnetohydrodynamic and collisionless regimes.
Main Results:
- The global magnetic reconnection rate is found to be independent of the Lundquist number.
- The distribution of fluxes within the plasmoids follows an inverse-square law.
- A finite probability exists for the formation of abnormally large plasmoids, capable of disrupting the plasmoid chain.
- A criterion for the transition from resistive magnetohydrodynamics (MHD) to the collisionless regime is established.
Conclusions:
- The proposed stochastic plasmoid chain model provides a framework for understanding resistive magnetic reconnection.
- The independence of the reconnection rate from the Lundquist number and the inverse-square flux distribution offer new insights into plasma dynamics.
- The potential for large plasmoid formation highlights a mechanism for abrupt events in astrophysical and laboratory plasmas.
- The derived criterion aids in distinguishing between different plasma regimes during reconnection.
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