The Atmospheric Response to High Nonthermal Electron Beam Fluxes in Solar Flares. I. Modeling the Brightest NUV Footpoints in the X1 Solar Flare of 2014 March 29

@article{Kowalski2017TheAR,
  title={The Atmospheric Response to High Nonthermal Electron Beam Fluxes in Solar Flares. I. Modeling the Brightest NUV Footpoints in the X1 Solar Flare of 2014 March 29},
  author={Adam F. Kowalski and Joel C. Allred and Adrian N. Daw and Gianna Cauzzi and Mats Carlsson},
  journal={The Astrophysical Journal},
  year={2017},
  volume={836},
  pages={12}
}
  • Adam F. Kowalski, Joel C. Allred, +2 authors Mats Carlsson
  • Published 2017
  • Physics
  • The Astrophysical Journal
  • The 2014 March 29 X1 solar flare (SOL20140329T17:48) produced bright continuum emission in the far- and near-ultraviolet (NUV) and highly asymmetric chromospheric emission lines, providing long-sought constraints on the heating mechanisms of the lower atmosphere in solar flares. We analyze the continuum and emission line data from the Interface Region Imaging Spectrograph (IRIS) of the brightest flaring magnetic footpoints in this flare. We compare the NUV spectra of the brightest pixels to new… CONTINUE READING

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