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Mathematics demonstrates that an ideally evolving magnetic field has an exponentially increasing sensitivity to non-ideal effects for all but truly exceptional evolutions.
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H. Ji and W. Daughton, Phase diagram for magnetic reconnection in heliophysical, astrophysical, and laboratory plasmas , Phys. Plasmas 18
2011
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2012
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2013
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2017
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P. Song, A model of the solar chromosphere: structure and internal circulation , Ap. J. 846
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A. H. Boozer, Why fast magnetic reconnection is so prevalent , J. Plasma Phys. 84
2018
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A. H. Boozer, Fast magnetic reconnection and the ideal evolution of a magnetic field , Phys. Plasmas 26
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