3D MHD flux emergence experiments: idealised models and coronal interactions:

Alan W. Hood, V. Archontis, David MacTaggart

Research output: Contribution to journalArticle

  • 22 Citations

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.
Original languageEnglish
Pages (from-to)3–31
Number of pages29
JournalSolar Physics
Volume278
Issue number1
DOIs
StatePublished - 2012

Fingerprint

magnetic fields
interactions
magnetic field
experiment
solar interior
shock heating
internal energy
heating
energy

Cite this

Hood, A. W., Archontis, V., & MacTaggart, D. (2012). 3D MHD flux emergence experiments: idealised models and coronal interactions: Solar Physics, 278(1), 3–31. DOI: 10.1007/s11207-011-9745-2

Hood, Alan W.; Archontis, V.; MacTaggart, David / 3D MHD flux emergence experiments : idealised models and coronal interactions:

In: Solar Physics, Vol. 278, No. 1, 2012, p. 3–31.

Research output: Contribution to journalArticle

@article{12ee51dc62aa4f588d8aeebf9d8efce9,
title = "3D MHD flux emergence experiments: idealised models and coronal interactions:",
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.",
author = "Hood, {Alan W.} and V. Archontis and David MacTaggart",
year = "2012",
doi = "10.1007/s11207-011-9745-2",
volume = "278",
pages = "3–31",
journal = "Solar Physics",
issn = "0038-0938",
publisher = "Springer Netherlands",
number = "1",

}

Hood, AW, Archontis, V & MacTaggart, D 2012, '3D MHD flux emergence experiments: idealised models and coronal interactions:' Solar Physics, vol 278, no. 1, pp. 3–31. DOI: 10.1007/s11207-011-9745-2

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 journalArticle

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 -

Hood AW, Archontis V, MacTaggart D. 3D MHD flux emergence experiments: idealised models and coronal interactions: Solar Physics. 2012;278(1):3–31. Available from, DOI: 10.1007/s11207-011-9745-2