The spectral difference between solar flare HXR coronal and footpoint sources due to wave-particle interactions (bibtex)
by I. G. Hannah, E. P. Kontar
Reference:
The spectral difference between solar flare HXR coronal and footpoint sources due to wave-particle interactions , I. G. Hannah, E. P. Kontar, Astronomy & Astrophysics, volume 529, 2011.
Bibtex Entry:
@ARTICLE{2011A&A...529A.109H,
   author = {{Hannah}, I.~G. and {Kontar}, E.~P.},
    title = "{The spectral difference between solar flare HXR coronal and footpoint sources due to wave-particle interactions}",
  journal = {\aap},
archivePrefix = "arXiv",
   eprint = {1103.2257},
 primaryClass = "astro-ph.SR",
 keywords = {Sun: corona, Sun: flares, Sun: X-rays, gamma rays},
     year = 2011,
    month = may,
   volume = 529,
      eid = {A109},
    pages = {A109},
      doi = {10.1051/0004-6361/201015710},
   adsurl = {http://adsabs.harvard.edu/abs/2011A%26A...529A.109H},
  adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}
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