NASA NTRS · 19900054452
Double-peaked electrostatic ion cyclotron harmonic waves
Abstract
Electrostatic H(+) cyclotron harmonic waves are often observed along the auroral field lines at altitudes of 1-3.5 R(E) by the Dynamics Explorer 1 satellite. A small fraction of these waves are found to have two peaks associated with each harmonic instead of one peak. The waves occur below the lower hybrid frequency and are usually relatively weak, about a factor of 4 smaller than typical electric field amplitudes of other H(+) cyclotron harmonic wave events. The double-peaked spectral signature is believed to be produced by Doppler shifts arising from the satellite velocity relative to the plasma rest frame. The waves were found to have wavelengths of the order of 300 m and phase velocities of the order of 150 km/s.
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Boardsen, S. A., Gurnett, D. A., Peterson, W. K.. 1990-07-01. Double-peaked electrostatic ion cyclotron harmonic waves. https://ntrs.nasa.gov/citations/19900054452
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