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 idealised, 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. © 2011 Springer Science+Business Media B.V.
3D MHD Flux Emergence Experiments: Idealised Models and Coronal Interactions / Hood, A.W., Archontis, V., Mactaggart, D.. - In: SOLAR PHYSICS. - ISSN 0038-0938. - 278:1(2012), pp. 3-31. [10.1007/s11207-011-9745-2]
3D MHD Flux Emergence Experiments: Idealised Models and Coronal Interactions
MacTaggart D.
2012-01-01
Abstract
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 idealised, 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. © 2011 Springer Science+Business Media B.V.I documenti in IRIS sono protetti da copyright e tutti i diritti sono riservati, salvo diversa indicazione
