Physics of Solar Prominences: II Magnetic Structure and Dynamics

Duncan Hendry Mackay; J Karpen; Jose-Luis Ballester; B Schmieder; G Aulanier

doi:10.1007/s11214-010-9628-0

Physics of Solar Prominences: II Magnetic Structure and Dynamics

Duncan Hendry Mackay, J Karpen, Jose-Luis Ballester, B Schmieder, G Aulanier

Applied Mathematics

Research output: Contribution to journal › Article › peer-review

Abstract

Observations and models of solar prominences are reviewed. We focus on non-eruptive prominences, and describe recent progress in four areas of prominence research: (1) magnetic structure deduced from observations and models, (2) the dynamics of prominence plasmas (formation and flows), (3) Magneto-hydrodynamic (MHD) waves in prominences and (4) the formation and large-scale patterns of the filament channels in which prominences are located. Finally, several outstanding issues in prominence research are discussed, along with observations and models required to resolve them.

Original language	English
Pages (from-to)	333-399
Journal	Space Science Reviews
Volume	151
Issue number	4
DOIs	https://doi.org/10.1007/s11214-010-9628-0
Publication status	Published - Apr 2010

Access to Document

10.1007/s11214-010-9628-0

Solar&Magnetospheric Plasma Theory PP/E1: Solar and Magnetospheric Plasma Theory
Neukirch, T. (PI), Hood, A. W. (CoI), Parnell, C. E. (CoI), Priest, E. (CoI), Roberts, B. (CoI) & Wright, A. N. (CoI)
PPARC - Now STFC
1/04/07 → 31/03/12
Project: Standard
PPARC FELOWSHIP-D MACKAY: Dynamic Solar Magnitude Fields
Mackay, D. H. (PI)
PPARC - Now STFC
1/10/04 → 30/09/09
Project: Standard

Cite this

@article{d8ec63c464e4482c82ac953663a9b3dc,

title = "Physics of Solar Prominences: II Magnetic Structure and Dynamics",

abstract = "Observations and models of solar prominences are reviewed. We focus on non-eruptive prominences, and describe recent progress in four areas of prominence research: (1) magnetic structure deduced from observations and models, (2) the dynamics of prominence plasmas (formation and flows), (3) Magneto-hydrodynamic (MHD) waves in prominences and (4) the formation and large-scale patterns of the filament channels in which prominences are located. Finally, several outstanding issues in prominence research are discussed, along with observations and models required to resolve them. ",

author = "Mackay, {Duncan Hendry} and J Karpen and Jose-Luis Ballester and B Schmieder and G Aulanier",

year = "2010",

month = apr,

doi = "10.1007/s11214-010-9628-0",

language = "English",

volume = "151",

pages = "333--399",

journal = "Space Science Reviews",

issn = "0038-6308",

publisher = "Springer",

number = "4",

}

TY - JOUR

T1 - Physics of Solar Prominences: II Magnetic Structure and Dynamics

AU - Mackay, Duncan Hendry

AU - Karpen, J

AU - Ballester, Jose-Luis

AU - Schmieder, B

AU - Aulanier, G

PY - 2010/4

Y1 - 2010/4

N2 - Observations and models of solar prominences are reviewed. We focus on non-eruptive prominences, and describe recent progress in four areas of prominence research: (1) magnetic structure deduced from observations and models, (2) the dynamics of prominence plasmas (formation and flows), (3) Magneto-hydrodynamic (MHD) waves in prominences and (4) the formation and large-scale patterns of the filament channels in which prominences are located. Finally, several outstanding issues in prominence research are discussed, along with observations and models required to resolve them.

AB - Observations and models of solar prominences are reviewed. We focus on non-eruptive prominences, and describe recent progress in four areas of prominence research: (1) magnetic structure deduced from observations and models, (2) the dynamics of prominence plasmas (formation and flows), (3) Magneto-hydrodynamic (MHD) waves in prominences and (4) the formation and large-scale patterns of the filament channels in which prominences are located. Finally, several outstanding issues in prominence research are discussed, along with observations and models required to resolve them.

U2 - 10.1007/s11214-010-9628-0

DO - 10.1007/s11214-010-9628-0

M3 - Article

SN - 0038-6308

VL - 151

SP - 333

EP - 399

JO - Space Science Reviews

JF - Space Science Reviews

IS - 4

ER -

Physics of Solar Prominences: II Magnetic Structure and Dynamics

Abstract

Access to Document

Fingerprint

Projects

Solar&Magnetospheric Plasma Theory PP/E1: Solar and Magnetospheric Plasma Theory

PPARC FELOWSHIP-D MACKAY: Dynamic Solar Magnitude Fields

Cite this