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- W2153939215 abstract "Within a MHD approach we find magnetic reconnection to progress in two entirely different ways. The first is well known: the laminar Sweet-Parker process. But a second, completely different and chaotic reconnection process is possible. This regime has properties of immediate practical relevance: (i) it is much faster, developing on scales of the order of the Alfvén time, and (ii) the areas of reconnection become distributed chaotically over a macroscopic region. The onset of the faster process is the formation of closed-circulation patterns where the jets going out of the reconnection regions turn around and force their way back in, carrying along copious amounts of magnetic flux." @default.
- W2153939215 created "2016-06-24" @default.
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- W2153939215 date "2008-06-09" @default.
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- W2153939215 title "Self-Feeding Turbulent Magnetic Reconnection on Macroscopic Scales" @default.
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- W2153939215 doi "https://doi.org/10.1103/physrevlett.100.235001" @default.
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