Bursts of large amplitude impulsive electric and magnetic field oscillation
s are a common feature observed from FAST when crossing the dayside auroral
oval at altitudes from 1500-2500 km. The oscillations have transverse ampl
itudes of up to 1 Vim and 100nT and exhibit a parallel electric field compo
nent with amplitudes which may be as large as 100mV/m. Calculation of E-1/B
-1 over 100 events yields an average value four times the local Alfven spee
d. The wave period is usually less than 0.25s with 'perpendicular wavelengt
hs' which average to 7.1 electron skin depths (c/omega(pe)similar to 80m).
Poynting flux calculations indicate predominately downward fluxes with magn
itude up 10(-2) Wm(-2) usually accompanied by a smaller upwards component.
Invariably these waves are accompanied by field-aligned fluxes of down goin
g and sometimes counterstreaming suprathermal electrons. Comparison with th
eoretical studies indicate that these observations are consistent with the
characteristics of a shear Alfven wave with k(perpendicular to)omega(pc)/c
propagating in the inertial dispersive regime and interfering with a reflec
ted component. However the observed large parallel electric field component
, if real, has yet to be explained.