Heating of the Magnetically Confined Corona Driven by Footpoint Shuffling: Theory and Observational Signatures. Rappazzo, A. AGU Fall Meeting Abstracts, December, 2015.
bibtex   
@ARTICLE{2015AGUFMSH54A..04R,
   author = {{Rappazzo}, A.~F.},
    title = "{Heating of the Magnetically Confined Corona Driven by Footpoint Shuffling: Theory and Observational Signatures}",
  journal = {AGU Fall Meeting Abstracts},
 keywords = {7526 Magnetic reconnection, SOLAR PHYSICS, ASTROPHYSICS, AND ASTRONOMY, 7807 Charged particle motion and acceleration, SPACE PLASMA PHYSICS, 7835 Magnetic reconnection, SPACE PLASMA PHYSICS, 7846 Plasma energization, SPACE PLASMA PHYSICS},
     year = 2015,
    month = dec,
   adsurl = {http://adsabs.harvard.edu/abs/2015AGUFMSH54A..04R},
  adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

Downloads: 0