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Solar Physics

, 294:124 | Cite as

Time-Dependent Two-Fluid Magnetohydrodynamic Model and Simulation of the Chromosphere

  • Qusai Al ShidiEmail author
  • Ofer Cohen
  • Paul Song
  • Jiannan Tu
Article

Abstract

The Sun’s chromosphere is a highly dynamic, partially ionized region where spicules (hot jets of plasma) form. Here we present a two-fluid MHD model to study the chromosphere, which includes ion–neutral interaction and frictional heating. Our simulation recovers a magnetic-canopy shape that forms quickly, but it is also quickly disrupted by the formation of a jet. Our simulation produces a shock self-consistently, where the jet is driven by the frictional heating, which is much greater than the ohmic heating. Thus, our simulation demonstrates that the jet could be driven purely by thermal effects due to ion–neutral collisions and not by magnetic reconnection. We plan to improve the model to include photo-chemical effects and radiation.

Keywords

Chromosphere, Models Jets 

Notes

Acknowledgments

We thank an unknown referee for useful comments and suggestions. O. Cohen was supported by NASA Living with a Star grant number NNX16AC11G. J. Tu and P. Song were supported by NSF grants AGS-1702134 and AGS-1559717.

Disclosure of Potential Conflicts of Interest

The authors declare that they have no conflicts of interest.

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Copyright information

© Springer Nature B.V. 2019

Authors and Affiliations

  1. 1.Climate and Space Science and EngineeringUniversity of MichiganAnn ArborUSA
  2. 2.Lowell Center for Space Science and TechnologyUniversity of Massachusetts LowellLowellUSA

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