Ijd. Craig et Rb. Fabling, EXACT-SOLUTIONS FOR STEADY-STATE, SPINE, AND FAN MAGNETIC RECONNECTION, The Astrophysical journal, 462(2), 1996, pp. 969-976
The problem of steady state, incompressible magnetic reconnection in t
hree dimensions is addressed. It is shown that exact reconnection solu
tions can be constructed by superposing nonlinear disturbances onto th
ree-dimensional magnetic X-points. There are two distinct families of
reconnection solutions. These can be understood in terms of the eigens
tructure of the null, that is, in terms of the ''spine'' curves and ''
fan'' surfaces that define the separatrices of the field. One family o
f solutions is driven by disturbances in the fan and involves quasi-cy
lindrical current structures aligned to the axis of the spine; the oth
er is associated with advection across the spine and a global current
sheet aligned to the fan. Although both spine and fan solutions reduce
to the two-dimensional analytic, shear-flow solutions of Craig & Hent
on, the three-dimensional spine current formulation allows far richer
reconnective current structures.