Static and Dynamic Modeling of a Solar Active Region

@article{Warren2007StaticAD,
  title={Static and Dynamic Modeling of a Solar Active Region},
  author={Harry P. Warren and Amy R. Winebarger},
  journal={The Astrophysical Journal},
  year={2007},
  volume={666},
  pages={1245-1255}
}
Recent hydrostatic simulations of solar active regions have shown that it is possible to reproduce both the total intensity and the general morphology of the high-temperature emission observed at soft X-ray wavelengths using static heating models. These static models, however, cannot account for the lower temperature emission. In addition, there is ample observational evidence that the solar corona is highly variable, indicating a significant role for dynamical processes in coronal heating… Expand

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