In this paper we present a theoretical framework for the Magnetic Reco
nnection Experiment (MRX) [M. Yamada et al., Bull. Am. Phys. Sec. 40,
1877 (1995)] in order to understand the basic physics of the experimen
t, including the effect of the external driving force, and the differe
nce between co-and counterhelicity cases of the experiment. The proble
m is reduced to a one-dimensional (1-D) resistive magnetohydrodynamic
(MHD) model. A special class of holonomic boundary conditions is defin
ed, under which a unique sequence of global equilibria can be obtained
, independent of the rate of reconnection. This enables one to break t
he whole problem into two parts: a global problem for the ideal region
, and a local problem for the resistive reconnection layer. The calcul
ations are then carried out and the global solution for the ideal regi
on is obtained in one particular case of holonomic constraints, the so
called ''constant force'' regime, for both the co- and counterhelicit
y cases. After the sequence of equilibria in the ideal region is found
, the problem of the rate of reconnection in the resistive reconnectio
n region is considered. This rate tells how fast the plasma proceeds t
hrough the sequence of global equilibria but does not affect the seque
nce itself. Based on a modified Sweet-Parker model for the reconnectio
n layer, the reconnection rate is calculated, and the difference betwe
en the co- and counterhelicity cases, as well as the role of the exter
nal forces is demonstrated. The results from the present analysis are
qualitatively consistent with the experimental data, predicting faster
reconnection rate for the counterhelicity merging and yielding a posi
tive correlation with external forcing. (C) 1996 American Institute of
Physics.