Using Pc5 pulsation events observed with the IMAGE magnetometer array, we d
emonstrate that mHz frequency field line resonances (FLRs) represent local
enhancements in the background Alfven continuum of field line eigenfrequenc
ies. By comparing resonance profiles for a typical event with the continuum
frequency profile determined using cross-phase techniques, we show that pu
lsation frequencies as low as 1-2 mHz can couple to FLRs on high latitude c
losed field lines. We also suggest that the transition to open field lines
on days of higher geomagnetic activity may lead to a breakdown in pulsation
characteristics at the highest latitudes of the IMAGE array. In addition,
we show evidence of the U-shaped diurnal variation in field line eigenfrequ
ency and suggest that this is primarily due to field line stretching, espec
ially on the magnetosphere flanks.