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

^*Corresponding author for this work

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

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
Pages (from-to)	760-763
Number of pages	4
Journal	AIP Conference Proceedings
Volume	1094
DOIs	https://doi.org/10.1063/1.3099226
Publication status	Published - 2009
Externally published	Yes
Event	15th Cambridge Workshop on Cool Stars, Stellar Systems and the Sun - St. Andrews, United Kingdom Duration: Jul 21 2008 → Jul 25 2008

Keywords

Coronae
Magnetohydrodynamics(mhd)
Plasmas
Rotation

ASJC Scopus subject areas

General Physics and Astronomy

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10.1063/1.3099226

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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 = "Coronae, Magnetohydrodynamics(mhd), Plasmas, Rotation",

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

year = "2009",

doi = "10.1063/1.3099226",

language = "English",

volume = "1094",

pages = "760--763",

journal = "AIP Conference Proceedings",

issn = "0094-243X",

publisher = "American Institute of Physics Publising LLC",

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

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TY - JOUR

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 - Coronae

KW - Magnetohydrodynamics(mhd)

KW - Plasmas

KW - Rotation

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DO - 10.1063/1.3099226

M3 - Conference article

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SN - 0094-243X

VL - 1094

SP - 760

EP - 763

JO - AIP Conference Proceedings

JF - AIP Conference Proceedings

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

Keywords

ASJC Scopus subject areas

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