Observationally driven 3D magnetohydrodynamics model of the solar corona above an active region

@article{Bourdin2013ObservationallyD3,
  title={Observationally driven 3D magnetohydrodynamics model of the solar corona above an active region},
  author={Ph.-A. Bourdin and Sven Bingert and Hardi Peter Max-Planck-Institut fur Sonnensystemforschung and Institut fur Theoretische Astrophysik and Universitat Gottingen},
  journal={Astronomy and Astrophysics},
  year={2013},
  volume={555}
}
  • Ph.-A. Bourdin, Sven Bingert, +2 authors Universitat Gottingen
  • Published 2013
  • Physics
  • Astronomy and Astrophysics
  • Institut fu¨r Astrophysik, Universita¨t Go¨ttingen, Friedrich-Hund-Platz 1, 37077 Go¨ttingen, GermanyReceived 29 January 2013 / Accepted 9 May 2013ABSTRACTAims. The goal is to employ a 3D magnetohydrodynamics (MHD) model including spectral synthesis to model the corona in anobserved solar active region. This will allow us to judge the merits of the coronal heating mechanism built into the 3D model.Methods.Photospheric observations of the magnetic field and horizon tal velocities in an active… CONTINUE READING

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