NON-AXISYMMETRIC MAGNETOSTATIC EQUILIBRIUM WITH WEAK TWISTED MAGNETIC FIELDS

The existence of the non-axisymmetrie magnetostatic equilibrium configuration was proved and the basic features of the fields were discussed. Observations show that the cosmic magnetic fields are often the configurations in three-dimensions, for example, the sunspot has the structures of bright and dark fibrils. In the viewpoint of theoretical analysis, the conclusion that the cosmic magnetic field should be symmetric in some sense may be changed if an applied gravity is introduced. Some good-resolution white light observations also show that the eonfigurations of sunspot