The tool used for this study is a numerical code which treats the plasma as
an incompressible fluid of low resistivity and which utilizes simplifying
assumptions on geometry. For a given set of "almost ideal magnetohydrodynam
ic (MHD) constraints" [T. H. Jensen, A. W. Leonard, R. J. La Haye, and M. S
. Chu, Phys. Fluids B 3, 1650 (1991)], the code can find equilibria which s
atisfy these constraints when boundary conditions and external currents are
specified. Thus, given an initial MHD equilibrium (without an island), and
thereby its constraints, the code can be used to find external currents ne
eded for establishing an equilibrium with the same constraints and an islan
d of specified width. The sign of these external currents determines whethe
r the island would grow or shrink if the external currents were removed. Th
us the code can provide information on nonlinear growth or decay, but not o
n the time scales involved. The two main points of the paper are (i) that t
he stability limit and saturated island width depend not only on the quanti
ty Delta' [H. P. Furth, J. Killeen, and M. N. Rosenbluth, Phys. Fluids 6, 4
59 (1963)] but also on the constraints imposed, and (ii) that a current den
sity gradient at the singular surface can drive a tearing mode nonlinearly
to a certain island width followed by a decrease until the island vanishes.
(C) 2001 American Institute of Physics.