This paper considers force-free equilibria in twisted magnetic Bur tub
es with helical symmetry. Such symmetry simplifies the force-free fiel
d condition to a pair of equations which are generalisations of the Gr
ad-Shafranov equations. A simple linear solution is given analytically
in terms of a Heun function, which exhibits several important aspects
of twisted flux tubes. The equilibrium equations impose a functional
relation between the axial field component and the flux function for t
he other two components, which can be used to establish current-sheer
formation when certain classes of flux tubes are twisted together. Imp
lications for magnetic energy release in the solar corona are discusse
d.