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Magnetic Reconnection

Null point

The reordering of field lines during magnetic reconnection plays an important part in many astrophysical and terrestrial plasma phenomena. Satellite measurements of a so-called null point during magnetic reconnection should help refine theoretical models of this process.

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Figure 1: Structure and flow (red) of field lines (blue) during magnetic reconnection in 2D.

References

  1. Priest, E. & Forbes, T. Magnetic Reconnection: MHD Theory and Applications. (Cambridge Univ. Press, New York, 2002).

    MATH  Google Scholar 

  2. Biskamp, D. Magnetic Reconnection in Plasmas. (Cambridge Univ. Press, New York, 2000).

    Book  Google Scholar 

  3. Xiao, C. J. et al. Nature Phys. 2, 478–483 (2006).

    Article  ADS  Google Scholar 

  4. Greene, J. M. J. Comp. Phys. 98, 194–198 (1992).

    Article  ADS  Google Scholar 

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Finn, J. Null point. Nature Phys 2, 445–446 (2006). https://doi.org/10.1038/nphys353

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  • DOI: https://doi.org/10.1038/nphys353

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