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Published online by Cambridge University Press: 13 March 2009
A solution to the Grad–Shafranov equation is obtained by expanding the MHD equilibrium functions in half-integer powers of the poloidal flux, about the magnetic axis. The poloidal angle dependence of the expansion coefficients is solved for, from a sequence of ordinary linear differential equations with constant coefficients. Flux conservation is achieved after calculating the inverse rotational transform, by requiring it to be invariant during the pressure rise.