Field Lines Twisting in a Noisy Corona: Implications for Energy Storage and Release, and Initiation of Solar Eruptions. Rappazzo, A., Velli, M., & Einaudi, G. \apj, 771:76, July, 2013.
doi  bibtex   
@ARTICLE{2013ApJ...771...76R,
   author = {{Rappazzo}, A.~F. and {Velli}, M. and {Einaudi}, G.},
    title = "{Field Lines Twisting in a Noisy Corona: Implications for Energy Storage and Release, and Initiation of Solar Eruptions}",
  journal = {\apj},
archivePrefix = "arXiv",
   eprint = {1301.7678},
 primaryClass = "astro-ph.SR",
 keywords = {magnetohydrodynamics: MHD, Sun: corona, Sun: coronal mass ejections: CMEs, Sun: magnetic topology, turbulence },
     year = 2013,
    month = jul,
   volume = 771,
      eid = {76},
    pages = {76},
      doi = {10.1088/0004-637X/771/2/76},
   adsurl = {http://adsabs.harvard.edu/abs/2013ApJ...771...76R},
  adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

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