3D MHD Flux Emergence Experiments: Idealized models and coronal interactions

Details 3D MHD Flux Emergence Experiments: Idealized models and coronal interactions 3D MHD Flux Emergence Experiments: Idealized models and coronal interactions

2011-03-18

arxiv.org/abs/1103.3685v1

Astronomy and Astrophysics

Astrophysics

Solar and Stellar Astrophysics

Review article, accepted for publication in Solar Physics

Scientific paper

This paper reviews some of the many 3D numerical experiments of the emergence of magnetic fields from the solar interior and the subsequent interaction with the pre-existing coronal magnetic field. The models described here are idealized, in the sense that the internal energy equation only involves the adiabatic, Ohmic and viscous shock heating terms. However, provided the main aim is to investigate the dynamical evolution, this is adequate. Many interesting observational phenomena are explained by these models in a self-consistent manner.

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