The Astrophysical Journal · 1984 · 338 citations · 0 references
Natural SciencesAstronomyPhysicsAstrophysicsElectromagnetismTheoretical AstronomyMagnetic FieldsMagnetohydrodynamicsSolar FlaresSolar Magnetic FieldsSolar PhysicsStellar Magnetic FieldsForce-free Magnetic FieldsMagnetic EnergyMagnetic Fields In Stellar AtmospheresMagnetic Free EnergySolar MagnetohydrodynamicsSolar X-ray FlaresStellar Magnetic Activity
Techniques for solving boundary value problems (BVP) for a force free magnetic field (FFF) in infinite space are presented. A priori inequalities are defined which must be satisfied by the force-free equations. It is shown that upper bounds may be calculated for the magnetic energy of the region provided the value of the magnetic normal component at the boundary of the region can be shown to decay sufficiently fast at infinity. The results are employed to prove a nonexistence theorem for the BVP for the FFF in the spatial region. The implications of the theory for modeling the origins of solar flares are discussed.