We present a class of one-dimensional, strictly neutral, Vlasov-Maxwell equilibrium distribution functions for force-free current sheets, with magnetic fields defined in terms of Jacobian elliptic functions, extending the results of Abraham-Shrauner [Phys. Plasmas 20, 102117 (2013)] to allow for non-uniform density and temperature profiles. To achieve this, we use an approach previously applied to the force-free Harris sheet by Kolotkov et al. [Phys. Plasmas 22, 112902 (2015)]. In one limit of the parameters, we recover the model of Kolotkov et al. [Phys. Plasmas 22, 112902 (2015)], while another limit gives a linear force-free field. We discuss conditions on the parameters such that the distribution functions are always positive and give e...
Current sheets in the collisionless solar wind usually have kinetic spatial scales. In-situ measurem...
A family of self-consistent collisionless distribution functions for the force-free Harris sheet is ...
Using the magnetohydrodynamic description, the evolution of a resistive plasma can be represented as...
The authors acknowledge the support of the Science and Technology Facilities Council via the consoli...
We present a first discussion and analysis of the physical properties of a new exact collisionless e...
So far, only one distribution function giving rise to a collisionless nonlinear force-free current s...
We consider the theory and application of a solution method for the inverse problem in collisionless...
Funding: STFC Consolidated Grant [ST/K000950/1] (OA, TN & FW) and a Doctoral Training Grant [ST/K502...
The kinetic model of a one-dimensional force-free current sheet (CS) developed recently by Harrison ...
We acknowledge the support of the Science and Technology Facilities Council via the consolidated gra...
Vlasov–Maxwell equilibria are described by the self-consistent solutions of the time-independent Max...
The work in this thesis focuses primarily on equilibrium and stability properties of collisionless c...
Current sheets are important for the structure and dynamics of many plasma systems. In space and ast...
In this thesis examples of translationally invariant one-dimensional (1D) Vlasov-Maxwell (VM) equili...
We calculate exact one-dimensional collisionless plasma equilibria for a continuum of flux tube mode...
Current sheets in the collisionless solar wind usually have kinetic spatial scales. In-situ measurem...
A family of self-consistent collisionless distribution functions for the force-free Harris sheet is ...
Using the magnetohydrodynamic description, the evolution of a resistive plasma can be represented as...
The authors acknowledge the support of the Science and Technology Facilities Council via the consoli...
We present a first discussion and analysis of the physical properties of a new exact collisionless e...
So far, only one distribution function giving rise to a collisionless nonlinear force-free current s...
We consider the theory and application of a solution method for the inverse problem in collisionless...
Funding: STFC Consolidated Grant [ST/K000950/1] (OA, TN & FW) and a Doctoral Training Grant [ST/K502...
The kinetic model of a one-dimensional force-free current sheet (CS) developed recently by Harrison ...
We acknowledge the support of the Science and Technology Facilities Council via the consolidated gra...
Vlasov–Maxwell equilibria are described by the self-consistent solutions of the time-independent Max...
The work in this thesis focuses primarily on equilibrium and stability properties of collisionless c...
Current sheets are important for the structure and dynamics of many plasma systems. In space and ast...
In this thesis examples of translationally invariant one-dimensional (1D) Vlasov-Maxwell (VM) equili...
We calculate exact one-dimensional collisionless plasma equilibria for a continuum of flux tube mode...
Current sheets in the collisionless solar wind usually have kinetic spatial scales. In-situ measurem...
A family of self-consistent collisionless distribution functions for the force-free Harris sheet is ...
Using the magnetohydrodynamic description, the evolution of a resistive plasma can be represented as...