Stationary Magnetohydrodynamic Models of Three-Dimensional Rigidly Rotating Magnetized Coronae

Nasser Al-Salti; Thomas Neukirch

doi:10.1063/1.3099226

Stationary Magnetohydrodynamic Models of Three-Dimensional Rigidly Rotating Magnetized Coronae

Nasser Al-Salti, Thomas Neukirch

School of Mathematics and Statistics

Research output: Chapter in Book/Report/Conference proceeding › Conference contribution

Abstract

Example solutions of a theory for stationary 3D non-potential solutions of the MHD equations (in the co-rotating frame of reference) are presented. As a first step we present solutions for the mathematically simpler case of a massive central cylinder, but the theory can also be applied to spherical bodies. The fundamental equation of the theory is linear and in the cylindrical case it can be solved using standard methods. Possible application is the structure of coronae of (fast) rotating stars.

Original language	English
Title of host publication	Cool stars, stellar systems and the sun
Editors	E. Stempels
Publisher	American Institute of Physics
Pages	760-763
Number of pages	4
ISBN (Print)	978-0-7354-0627-8
DOIs	https://doi.org/10.1063/1.3099226
Publication status	Published - 2009
Event	15th Cambridge Workshop on Cool Stars, Stellar Systems and the Sun - St Andrews, St Andrews, United Kingdom Duration: 21 Jul 2008 → 25 Jul 2008

Publication series

Name	AIP Conference Proceedings
Volume	1094
ISSN (Print)	0094-243X

Conference

Conference	15th Cambridge Workshop on Cool Stars, Stellar Systems and the Sun
Country/Territory	United Kingdom
City	St Andrews
Period	21/07/08 → 25/07/08

Keywords

Stars: coronae
rotation
Magnetohydrodynamics (MHD)
Plasmas

Access to Document

10.1063/1.3099226

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

Cite this

@inproceedings{b9f23505e7924f94bbad9a7252d33709,

title = "Stationary Magnetohydrodynamic Models of Three-Dimensional Rigidly Rotating Magnetized Coronae",

abstract = "Example solutions of a theory for stationary 3D non-potential solutions of the MHD equations (in the co-rotating frame of reference) are presented. As a first step we present solutions for the mathematically simpler case of a massive central cylinder, but the theory can also be applied to spherical bodies. The fundamental equation of the theory is linear and in the cylindrical case it can be solved using standard methods. Possible application is the structure of coronae of (fast) rotating stars.",

keywords = "Stars: coronae, rotation, Magnetohydrodynamics (MHD), Plasmas",

author = "Nasser Al-Salti and Thomas Neukirch",

year = "2009",

doi = "10.1063/1.3099226",

language = "English",

isbn = "978-0-7354-0627-8 ",

series = "AIP Conference Proceedings",

publisher = "American Institute of Physics",

pages = "760--763",

editor = "E. Stempels",

booktitle = "Cool stars, stellar systems and the sun",

address = "United States",

note = "15th Cambridge Workshop on Cool Stars, Stellar Systems and the Sun ; Conference date: 21-07-2008 Through 25-07-2008",

}

Al-Salti, N & Neukirch, T 2009, Stationary Magnetohydrodynamic Models of Three-Dimensional Rigidly Rotating Magnetized Coronae. in E Stempels (ed.), Cool stars, stellar systems and the sun. AIP Conference Proceedings, vol. 1094, American Institute of Physics, pp. 760-763, 15th Cambridge Workshop on Cool Stars, Stellar Systems and the Sun, St Andrews, United Kingdom, 21/07/08. https://doi.org/10.1063/1.3099226

Stationary Magnetohydrodynamic Models of Three-Dimensional Rigidly Rotating Magnetized Coronae. / Al-Salti, Nasser; Neukirch, Thomas.
Cool stars, stellar systems and the sun. ed. / E. Stempels. American Institute of Physics, 2009. p. 760-763 (AIP Conference Proceedings; Vol. 1094).

Research output: Chapter in Book/Report/Conference proceeding › Conference contribution

TY - GEN

T1 - Stationary Magnetohydrodynamic Models of Three-Dimensional Rigidly Rotating Magnetized Coronae

AU - Al-Salti, Nasser

AU - Neukirch, Thomas

PY - 2009

Y1 - 2009

N2 - Example solutions of a theory for stationary 3D non-potential solutions of the MHD equations (in the co-rotating frame of reference) are presented. As a first step we present solutions for the mathematically simpler case of a massive central cylinder, but the theory can also be applied to spherical bodies. The fundamental equation of the theory is linear and in the cylindrical case it can be solved using standard methods. Possible application is the structure of coronae of (fast) rotating stars.

AB - Example solutions of a theory for stationary 3D non-potential solutions of the MHD equations (in the co-rotating frame of reference) are presented. As a first step we present solutions for the mathematically simpler case of a massive central cylinder, but the theory can also be applied to spherical bodies. The fundamental equation of the theory is linear and in the cylindrical case it can be solved using standard methods. Possible application is the structure of coronae of (fast) rotating stars.

KW - Stars: coronae

KW - rotation

KW - Magnetohydrodynamics (MHD)

KW - Plasmas

U2 - 10.1063/1.3099226

DO - 10.1063/1.3099226

M3 - Conference contribution

SN - 978-0-7354-0627-8

T3 - AIP Conference Proceedings

SP - 760

EP - 763

BT - Cool stars, stellar systems and the sun

A2 - Stempels, E.

PB - American Institute of Physics

T2 - 15th Cambridge Workshop on Cool Stars, Stellar Systems and the Sun

Y2 - 21 July 2008 through 25 July 2008

ER -

Stationary Magnetohydrodynamic Models of Three-Dimensional Rigidly Rotating Magnetized Coronae

Abstract

Publication series

Conference

Keywords

Access to Document

Fingerprint

Projects

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

Cite this