The high time resolution observations by the Fast Auroral Snapshot satellit
e resolve burst-like electrons and nonmonotonic ion dispersion in the cusp
region. Electric field data from a dawn-dusk cusp crossing show that the DC
electric field has small-scale variations superimposed on a large-scale pa
ttern. The large-scale DC electric field variations are well correlated wit
h the large-scale perturbation magnetic field, indicating a field-aligned c
urrent system that reflects a relatively homogenous conductivity. Ion struc
tures best correlate with the perturbed magnetic field and the large-scale
electric field. The burst-like precipitating electrons are correlated with
the small-scale electric field variations, which are most easily explained
as propagating Alfven waves. We also found that the observed ion structures
result from the spacecraft crossing the flow streamlines, each of which ha
s its own individual history of dayside reconnection. The magnetosheath ion
structures therefore contain information of both the spatial and temporal
variations of dayside reconnection.