Filament Channels: Isolated Laboratories of Plasma Heating in the Solar Corona. Panasenco, O. & Velli, M. AGU Fall Meeting Abstracts, December, 2015.
bibtex   
@ARTICLE{2015AGUFMSH13C2454P,
   author = {{Panasenco}, O. and {Velli}, M.},
    title = "{Filament Channels: Isolated Laboratories of Plasma Heating in the Solar Corona}",
  journal = {AGU Fall Meeting Abstracts},
 keywords = {7507 Chromosphere, SOLAR PHYSICS, ASTROPHYSICS, AND ASTRONOMY, 7509 Corona, SOLAR PHYSICS, ASTROPHYSICS, AND ASTRONOMY, 7511 Coronal holes, SOLAR PHYSICS, ASTROPHYSICS, AND ASTRONOMY, 7827 Kinetic and MHD theory, SPACE PLASMA PHYSICS},
     year = 2015,
    month = dec,
   adsurl = {http://adsabs.harvard.edu/abs/2015AGUFMSH13C2454P},
  adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

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