High bandwidth electric field waveform measurements on a recent auroral sounding rocket reveal structured whistler mode signals at 400--800 kHz. These are observed intermittently between 300 and 500 km with spectral densities 0--10 dB above the detection threshold of 1.5¿10-11 V2/m2 Hz. The lack of correlation with local particle measurements suggests a remote source. The signals are composed of discrete structures, in one case having bandwidths of about 10 kHz and exhibiting rapid frequency variations of the order of 200 kHz per 100 ms. In one case, emissions near the harmonic of the whistler mode signals are detected simultaneously. Current theories of auroral zone whistler mode emissions have not been applied to explain quantitatively the fine structure of these signals, which resemble auroral kilometric radiation (AKR) rather than auroral hiss. ¿ 1999 American Geophysical Union