Large-scale simulations of solar type III radio bursts: flux density, drift rate, duration, and bandwidth (bibtex)
by H. Ratcliffe, E. P. Kontar, H. A. S. Reid
Reference:
Large-scale simulations of solar type III radio bursts: flux density, drift rate, duration, and bandwidth , H. Ratcliffe, E. P. Kontar, H. A. S. Reid, Astronomy & Astrophysics, volume 572, 2014.
Bibtex Entry:
@ARTICLE{2014A&A...572A.111R,
   author = {{Ratcliffe}, H. and {Kontar}, E.~P. and {Reid}, H.~A.~S.},
    title = "{Large-scale simulations of solar type III radio bursts: flux density, drift rate, duration, and bandwidth}",
  journal = {\aap},
archivePrefix = "arXiv",
   eprint = {1410.2410},
 primaryClass = "astro-ph.SR",
 keywords = {Sun: particle emission, Sun: radio radiation, Sun: flares},
     year = 2014,
    month = dec,
   volume = 572,
      eid = {A111},
    pages = {A111},
      doi = {10.1051/0004-6361/201423731},
   adsurl = {http://adsabs.harvard.edu/abs/2014A%26A...572A.111R},
  adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}
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