Diagnosing the Source Region of a Solar Burst on 26 September 2011 by Using Microwave Type-III Pairs. Tan, B., Karlický, M., Mészárosová, H., Kashapova, L., Huang, J., Yan, Y., & Kontar, E. \solphys, 291:2407-2418, October, 2016.
doi  bibtex   
@ARTICLE{2016SoPh..291.2407T,
   author = {{Tan}, B.~L. and {Karlick{\'y}}, M. and {M{\'e}sz{\'a}rosov{\'a}}, H. and
	{Kashapova}, L. and {Huang}, J. and {Yan}, Y. and {Kontar}, E.~P.
	},
    title = "{Diagnosing the Source Region of a Solar Burst on 26 September 2011 by Using Microwave Type-III Pairs}",
  journal = {\solphys},
archivePrefix = "arXiv",
   eprint = {1606.05410},
 primaryClass = "astro-ph.SR",
 keywords = {Sun: microwave emission, Sun: magnetic reconnection, Sun: flares},
     year = 2016,
    month = oct,
   volume = 291,
    pages = {2407-2418},
      doi = {10.1007/s11207-016-0986-y},
   adsurl = {http://adsabs.harvard.edu/abs/2016SoPh..291.2407T},
  adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

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