Exact self-consistent solutions of the magnetohydrostatic equations in three dimensions with a nonlinear relationship between the magnetic field and the current density are presented. The derivation is carried out in Cartesian coordinates including a constant gravitational force pointing into the negative z-direction. Out of several solution classes only one has an arcade-like magnetic field topology. This solution class is investigated further and two examples are shown for specific choices of the free functions and parameters which the solution class has.</p
Context. Solutions of the magnetohydrostatic (MHS) equations are very important for modelling astrop...
Details are presented of the PIES code, which uses a nonvariational algorithm for calculating fully ...
The formation of electric current sheets in a high-conductivity three-dimensional plasma configurati...
A new mathematical formulation for calculating a special class of self-consistent three-dimensional ...
A new mathematical procedure is presented to calculate special self-consistent three-dimensional ana...
We present new analytical three-dimensional solutions of the magnetohydrostatic equations, which are...
Context. Solutions of the magnetohydrostatic (MHS) equations are very important for modelling astrop...
Context. Solutions of the magnetohydrostatic (MHS) equations are very important for modelling astrop...
Context. Solutions of the magnetohydrostatic (MHS) equations are very important for modelling astrop...
We present three-dimensional (3D) solutions of the magnetohydrostatic equations in the co-rotating f...
Context. Magnetohydrostatic (MHS) equilibria are often used to model astrophysical plasmas, for exam...
Context. Magnetohydrostatic (MHS) equilibria are often used to model astrophysical plasmas, for exam...
Context. Magnetohydrostatic (MHS) equilibria are often used to model astrophysical plasmas, for exam...
Context. Magnetohydrostatic (MHS) equilibria are often used to model astrophysical plasmas, for exam...
We present the Green's function method for a special class of linear self-consistent three-dimension...
Context. Solutions of the magnetohydrostatic (MHS) equations are very important for modelling astrop...
Details are presented of the PIES code, which uses a nonvariational algorithm for calculating fully ...
The formation of electric current sheets in a high-conductivity three-dimensional plasma configurati...
A new mathematical formulation for calculating a special class of self-consistent three-dimensional ...
A new mathematical procedure is presented to calculate special self-consistent three-dimensional ana...
We present new analytical three-dimensional solutions of the magnetohydrostatic equations, which are...
Context. Solutions of the magnetohydrostatic (MHS) equations are very important for modelling astrop...
Context. Solutions of the magnetohydrostatic (MHS) equations are very important for modelling astrop...
Context. Solutions of the magnetohydrostatic (MHS) equations are very important for modelling astrop...
We present three-dimensional (3D) solutions of the magnetohydrostatic equations in the co-rotating f...
Context. Magnetohydrostatic (MHS) equilibria are often used to model astrophysical plasmas, for exam...
Context. Magnetohydrostatic (MHS) equilibria are often used to model astrophysical plasmas, for exam...
Context. Magnetohydrostatic (MHS) equilibria are often used to model astrophysical plasmas, for exam...
Context. Magnetohydrostatic (MHS) equilibria are often used to model astrophysical plasmas, for exam...
We present the Green's function method for a special class of linear self-consistent three-dimension...
Context. Solutions of the magnetohydrostatic (MHS) equations are very important for modelling astrop...
Details are presented of the PIES code, which uses a nonvariational algorithm for calculating fully ...
The formation of electric current sheets in a high-conductivity three-dimensional plasma configurati...