MAGNETIC AND ELECTRIC-FIELD WAVES IN SLOW SHOCKS OF THE DISTANT GEOMAGNETIC TAIL - ISEE-3 OBSERVATIONS

During the first pass through the distant geomagnetic tail by ISEE 3 t he slow shocks encountered on February 2 and 11, 1983, provide particu larly clear examples of the magnetic field and plasma wave properties of the shock transition. The Magnetic ramp contains transverse polariz ed magnetic field oscillations with frequencies just below the ion cyc lotron frequency and amplitudes of 2-4 nT. These waves are plausibly g enerated by the electromagnetic ion/ion cyclotron instability predicte d by Winske and Omidi (1990). The electric field plasma waves within t he shock ramp exhibit two spectral peaks. A midfrequency emission occu rs near the ion plasma frequency and electron cyclotron frequency but well below the maximum Doppler shift frequency for electrostatic waves . The midfrequency waves extend into the upstream region where the spe ctral peak occurs at a slightly higher frequency. A new high-frequency emission with frequencies between the maximum Doppler shift frequency and the electron plasma frequency occurs throughout the downstream re gion. This emission disappears at the start of the magnetic ramp and i s replaced upstream by electron plasma oscillations. The high-frequenc y emissions are clearly polarized parallel to the magnetic field. The polarization of the midfrequency waves is less certain; both parallel and a fairly broad angular distribution about the parallel electric fi elds are consistent with the measurements.