Imaging Spectroscopy of Type U and J Solar Radio Bursts with LOFAR

@article{Reid2017ImagingSO,
  title={Imaging Spectroscopy of Type U and J Solar Radio Bursts with LOFAR},
  author={Hamish A. S. Reid and Eduard P. Kontar},
  journal={arXiv: Solar and Stellar Astrophysics},
  year={2017}
}
  • H. Reid, E. Kontar
  • Published 22 June 2017
  • Physics
  • arXiv: Solar and Stellar Astrophysics
Radio U-bursts and J-bursts are signatures of electron beams propagating along magnetic loops confined to the corona. The more commonly observed type III radio bursts are signatures of electron beams propagating along magnetic loops that extend into interplanetary space. Given the prevalence of solar magnetic flux to be closed in the corona, it is an outstanding question why type III bursts are more frequently observed than U-bursts or J-bursts. We use LOFAR imaging spectroscopy between 30-80… 

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