Grant numbers: Science and Technology Facilities Council via Doctoral Training Grant [ST/K502327/1], Consolidated Grant [ST/K000950/1] and Consolidated Grant [ST/N000609/1].We present a new approach to the theory of magnetohydrodynamic equilibria with anisotropic pressure, magnetic shear and translational/rotational invariance. This approach involves combining two existing formalisms in order to eliminate their individual weaknesses. The theoretical aspects of the method are explored in detail along with numerical solutions which make use of the method. Eventually, this method could be applied to model various plasma systems, such as planetary magnetospheres.Publisher PDFPeer reviewe
The ellipticity criteria for the partial differential equations of axisymmetric single-fluid and Hal...
[1] In order to better describe the space plasmas where pressure anisotropy has prominent effects, w...
[1] In order to better describe the space plasmas where pressure anisotropy has prominent effects, w...
Funding: STFC Doctoral Training Grant ST/K502327/1 (Jonathan Hodgson) and STFC Consolidated Grant ST...
In this thesis we discuss the theory of symmetric MHD equilibria with anisotropic pressure. More sp...
In many astrophysical plasmas, the Coulomb collision is insufficient to maintain an isotropic temper...
We present an improved formalism for translationally invariant magnetohydrodynamic equilibria with a...
It is well known that in many cases the dynamics of a magnetized plasma involve a very large number ...
The plasma flow past a blunt obstacle in an ideal magnetohydrodynamic (MHD) model is studied, taking...
Peer Reviewedhttp://deepblue.lib.umich.edu/bitstream/2027.42/95331/1/jgra22024.pd
3D equilibria with an anisotropic pressure component in the large helical device are analyzed with r...
3D equilibria with an anisotropic pressure component in the large helical device are analyzed with r...
The present generation of global 3D magnetohydrodynamic (MHD) simulations of the Sun-Earth environme...
We present an extension of the multi-region relaxed magnetohydrodynamics (MRxMHD) equilibrium model...
The present generation of global 3D magnetohydrodynamic (MHD) simulations of the Sun-Earth environme...
The ellipticity criteria for the partial differential equations of axisymmetric single-fluid and Hal...
[1] In order to better describe the space plasmas where pressure anisotropy has prominent effects, w...
[1] In order to better describe the space plasmas where pressure anisotropy has prominent effects, w...
Funding: STFC Doctoral Training Grant ST/K502327/1 (Jonathan Hodgson) and STFC Consolidated Grant ST...
In this thesis we discuss the theory of symmetric MHD equilibria with anisotropic pressure. More sp...
In many astrophysical plasmas, the Coulomb collision is insufficient to maintain an isotropic temper...
We present an improved formalism for translationally invariant magnetohydrodynamic equilibria with a...
It is well known that in many cases the dynamics of a magnetized plasma involve a very large number ...
The plasma flow past a blunt obstacle in an ideal magnetohydrodynamic (MHD) model is studied, taking...
Peer Reviewedhttp://deepblue.lib.umich.edu/bitstream/2027.42/95331/1/jgra22024.pd
3D equilibria with an anisotropic pressure component in the large helical device are analyzed with r...
3D equilibria with an anisotropic pressure component in the large helical device are analyzed with r...
The present generation of global 3D magnetohydrodynamic (MHD) simulations of the Sun-Earth environme...
We present an extension of the multi-region relaxed magnetohydrodynamics (MRxMHD) equilibrium model...
The present generation of global 3D magnetohydrodynamic (MHD) simulations of the Sun-Earth environme...
The ellipticity criteria for the partial differential equations of axisymmetric single-fluid and Hal...
[1] In order to better describe the space plasmas where pressure anisotropy has prominent effects, w...
[1] In order to better describe the space plasmas where pressure anisotropy has prominent effects, w...