Origins of Rolling, Twisting, and Non-radial Propagation of Eruptive Solar Events. Panasenco, O., Martin, S., Velli, M., & Vourlidas, A. \solphys, 287:391-413, October, 2013.
doi  bibtex   
@ARTICLE{2013SoPh..287..391P,
   author = {{Panasenco}, O. and {Martin}, S.~F. and {Velli}, M. and {Vourlidas}, A.
	},
    title = "{Origins of Rolling, Twisting, and Non-radial Propagation of Eruptive Solar Events}",
  journal = {\solphys},
archivePrefix = "arXiv",
   eprint = {1211.1376},
 primaryClass = "astro-ph.SR",
 keywords = {Coronal mass ejections, low coronal signatures, Coronal mass ejections, initiation and propagation, Magnetic fields, corona, Coronal holes, prominences, formation and evolution, Filaments},
     year = 2013,
    month = oct,
   volume = 287,
    pages = {391-413},
      doi = {10.1007/s11207-012-0194-3},
   adsurl = {http://adsabs.harvard.edu/abs/2013SoPh..287..391P},
  adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

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