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

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3D MHD Flux emergence experiments : idealised models and coronal interactions. / Hood, A.W.; Archontis, V.; Mactaggart, David.

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

Research output: Contribution to journal › Journal article › Research › peer-review

Harvard

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. https://doi.org/10.1007/s11207-011-9745-2

APA

Hood, A. W., Archontis, V., & Mactaggart, D. (2012). 3D MHD Flux emergence experiments: idealised models and coronal interactions. Solar Physics, 278(1), 3-31. https://doi.org/10.1007/s11207-011-9745-2

Vancouver

Hood AW, Archontis V, Mactaggart D. 3D MHD Flux emergence experiments: idealised models and coronal interactions. Solar Physics. 2012;278(1):3-31. https://doi.org/10.1007/s11207-011-9745-2

Author

Hood, A.W. ; Archontis, V. ; Mactaggart, David. / 3D MHD Flux emergence experiments : idealised models and coronal interactions. In: Solar Physics. 2012 ; Vol. 278, No. 1. pp. 3-31.

Bibtex

@article{2e8a9cca6ed345198e72c09a97faac35,
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 = "A.W. Hood and V. Archontis and David Mactaggart",
year = "2012",
doi = "10.1007/s11207-011-9745-2",
language = "English",
volume = "278",
pages = "3--31",
journal = "Solar Physics",
issn = "0038-0938",
publisher = "Springer",
number = "1",

}

RIS

TY - JOUR

T1 - 3D MHD Flux emergence experiments

T2 - idealised models and coronal interactions

AU - Hood, A.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 - Journal article

VL - 278

SP - 3

EP - 31

JO - Solar Physics

JF - Solar Physics

SN - 0038-0938

IS - 1

ER -

ID: 49733356