Coronal pseudostreamers: Source of fast or slow solar wind?. Panasenco, O. & Velli, M. Solar Wind 13, 1539:50-53, June, 2013.
doi  bibtex   
@ARTICLE{2013AIPC.1539...50P,
   author = {{Panasenco}, O. and {Velli}, M.},
    title = "{Coronal pseudostreamers: Source of fast or slow solar wind?}",
  journal = {Solar Wind 13},
archivePrefix = "arXiv",
   eprint = {1211.6171},
 primaryClass = "astro-ph.SR",
 keywords = {solar corona, solar magnetism, solar prominences, solar wind, Solar wind plasma, sources of solar wind, Electric and magnetic fields solar magnetism, Corona, Prominence eruptions, Particle emission solar wind},
     year = 2013,
    month = jun,
   volume = 1539,
    pages = {50-53},
      doi = {10.1063/1.4810987},
   adsurl = {http://adsabs.harvard.edu/abs/2013AIPC.1539...50P},
  adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

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