Using Coronal Cells to Infer the Magnetic Field Structure and Chirality of Filament Channels. Sheeley, Martin, S., Panasenco, O., & Warren, H. \apj, 772:88, August, 2013.
doi  bibtex   
@ARTICLE{2013ApJ...772...88S,
   author = {{Sheeley}, Jr., N.~R. and {Martin}, S.~F. and {Panasenco}, O. and 
	{Warren}, H.~P.},
    title = "{Using Coronal Cells to Infer the Magnetic Field Structure and Chirality of Filament Channels}",
  journal = {\apj},
archivePrefix = "arXiv",
   eprint = {1306.2273},
 primaryClass = "astro-ph.SR",
 keywords = {magnetic fields, Sun: corona, Sun: filaments, prominences, Sun: UV radiation },
     year = 2013,
    month = aug,
   volume = 772,
      eid = {88},
    pages = {88},
      doi = {10.1088/0004-637X/772/2/88},
   adsurl = {http://adsabs.harvard.edu/abs/2013ApJ...772...88S},
  adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

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