The IESP experiment implemented onboard the Interball auroral probe me
asures the six components (3B, 3E) of the waves in the ULF range: 0.1-
10 Hz and from time to time 0-30 Hz. Two different kinds of waves have
been observed in the auroral region at altitudes between 10 000 and 2
0 000 km: (1) electrostatic emissions which consist of quasi-monochrom
atic structures with frequencies above the oxygen gyrofrequency, super
imposed on a wide band signal interpreted as a Doppler broadening, (2)
electromagnetic wide band spectrum fluctuations. These emissions are
interpreted as current-driven electromagnetic or electrostatic ion cyc
lotron waves. The electromagnetic/electrostatic character is controlle
d by the plasma parameter beta(i) and by the O+ concentration.