We present detailed calculations and results for a model case of two-d
imensional small distortions of static, current-free equilibrium aroun
d a null-line magnetic configuration. This setup has been studied for
fast energy release in flares, but has not been studied before in the
context of the magnetic energy buildup that precedes the flare. Our an
alytical results are new because they include gas pressure and provide
explicit formulae for the expressions of all quantities (and especial
ly the electric current) and energy storage as functions of the values
of boundary conditions. A general solution is shown as a combination
of eigenfunctions, with coefficients resulting from the boundary condi
tions. These boundary conditions are given in terms of any arbitrary p
lasma acceleration at a boundary enclosing the domain we study. The ap
proach used here studies the MHD evolution of the electric current and
plasma density variations driven by external forces. We find that bot
h pressure and Lorentz forces are important, and that their boundary v
alues select between a wide range of solutions, many of which have bee
n found previously in numerical simulations. Most of the modes we find
display strong current sheets, velocities, and pressure variations at
the separatrices. Also we find that Joule and other dissipative terms
are not important for typical cases, except at an extremely narrow in
ner core, and near the separatrices. We discuss our results and their
relationship to numerical MHD simulations.