  A combination of analytical calculations and vectormagnetogram data are
utilized to develop a non-axisymmetric non-force-free magnetic field and asses
its viability in describing solar active regions. For the purpose, we construct
a local spherical shell where a planar surface, tangential to the inner sphere,
represents a Cartesian cutout of an active region. The magnetic field defined
on the surface is then correlated with magnetograms. The analysis finds the
non-axisymmetric non-force-free magnetic field, obtained by a superposition of
two linear-force-free fields, correlates reasonably well with magnetograms.
