The effect of the ponderomotive force (PF) on the temporal evolution o
f shear Alfven field line resonances (FLRs) is considered for a magnet
ic dipole geometry appropriate to the Earth's magnetosphere. We derive
a set of equations which describes the coupling of shear Alfven and s
low mode waves and show that in a dipole field, the PF initiates a spe
ctrum of standing slow mode waves, rather than just the fundamental mo
de that arises in a Cartesian box model magnetosphere. Magnetic field
aligned slow mode density perturbations lead to a nonlinear temporal p
hase shift between the compressional driver and shear Alfven wave. Thi
s results in nonlinear saturation of the wave fields of FLRs and may o
ccur well in advance of linear saturation as a result of ionospheric d
issipation. We derive expressions for the nonlinear frequency shifts c
aused by the slow mode spectrum and determine the timescale for nonlin
ear saturation of the shear Alfven wave fields. Finally, we compare ou
r results with previous estimates made in a box model magnetosphere an
d show that our main conclusions remain valid.