Abstract
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.
Original language | English |
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Pages (from-to) | 847-856 |
Number of pages | 10 |
Journal | Astronomy & Astrophysics |
Volume | 325 |
Publication status | Published - Sept 1997 |
Keywords
- magnetohydrodynamics
- magnetic fields
- plasmas
- Sun: magnetic fields
- Sun: corona
- stars: magnetic fields
- ELECTRIC-CURRENT SYSTEMS
- MAGNETOSTATIC ATMOSPHERES
- 3-DIMENSIONAL STRUCTURES
- MAGNETOHYDRODYNAMIC EQUILIBRIA
- MAGNETOTAIL THEORY
- FIELD LINES
- FORCE