The Parker Scenario for Coronal Heating as an MHD Turbulence Problem. Rappazzo, A., Velli, M., & Einaudi, G. In Howe, R., Komm, R., Balasubramaniam, K., & Petrie, G., editors, Subsurface and Atmospheric Influences on Solar Activity, volume 383, of Astronomical Society of the Pacific Conference Series, pages 353, 2008.
bibtex   
@INPROCEEDINGS{2008ASPC..383..353R,
   author = {{Rappazzo}, A.~F. and {Velli}, M. and {Einaudi}, G.},
    title = "{The Parker Scenario for Coronal Heating as an MHD Turbulence Problem}",
booktitle = {Subsurface and Atmospheric Influences on Solar Activity},
     year = 2008,
   series = {Astronomical Society of the Pacific Conference Series},
   volume = 383,
archivePrefix = "arXiv",
   eprint = {1002.2631},
 primaryClass = "astro-ph.SR",
   editor = {{Howe}, R. and {Komm}, R.~W. and {Balasubramaniam}, K.~S. and 
	{Petrie}, G.~J.~D.},
    pages = {353},
   adsurl = {http://adsabs.harvard.edu/abs/2008ASPC..383..353R},
  adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

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