Abstract
| Original language | English |
|---|---|
| Pages (from-to) | 3–31 |
| Number of pages | 29 |
| Journal | Solar Physics |
| Volume | 278 |
| Issue number | 1 |
| DOIs | |
| State | Published - 2012 |
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3D MHD flux emergence experiments : idealised models and coronal interactions: / Hood, Alan W.; Archontis, V.; MacTaggart, David.
In: Solar Physics, Vol. 278, No. 1, 2012, p. 3–31.Research output: Contribution to journal › Article
TY - JOUR
T1 - 3D MHD flux emergence experiments
T2 - Solar Physics
AU - Hood,Alan W.
AU - Archontis,V.
AU - MacTaggart,David
PY - 2012
Y1 - 2012
N2 - 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.
AB - 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.
U2 - 10.1007/s11207-011-9745-2
DO - 10.1007/s11207-011-9745-2
M3 - Article
VL - 278
SP - 3
EP - 31
JO - Solar Physics
JF - Solar Physics
SN - 0038-0938
IS - 1
ER -