Solar Coronal Jets: Observations, Theory, and Modeling

@article{Raouafi2016SolarCJ,
  title={Solar Coronal Jets: Observations, Theory, and Modeling},
  author={N. E. Raouafi and S. Patsourakos and E. Pariat and P. R. Young and A. C. Sterling and A. Savcheva and M. Shimojo and F. Moreno-Insertis and C. R. DeVore and V. Archontis and T. T{\"o}r{\"o}k and H. Mason and W. Curdt and K. Meyer and K. Dalmasse and Y. Matsui},
  journal={Space Science Reviews},
  year={2016},
  volume={201},
  pages={1-53}
}
Coronal jets represent important manifestations of ubiquitous solar transients, which may be the source of significant mass and energy input to the upper solar atmosphere and the solar wind. While the energy involved in a jet-like event is smaller than that of “nominal” solar flares and coronal mass ejections (CMEs), jets share many common properties with these phenomena, in particular, the explosive magnetically driven dynamics. Studies of jets could, therefore, provide critical insight for… CONTINUE READING

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