The role of plasma wave turbulence in the formation of shock waves in collisionless plasmas

Details The role of plasma wave turbulence in the formation of shock waves in collisionless plasmas The role of plasma wave turbulence in the formation of shock waves in collisionless plasmas

Sep 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987iowa.rept.....m&link_type=abstract

Final Report Iowa Univ., Iowa City. Dept. of Physics and Astronomy.

Astronomy and Astrophysics

Astronomy

Acoustic Emission, Bow Waves, Collisionless Plasmas, Electromagnetic Noise, Electron Plasma, Ion Emission, Low Frequencies, Plasma Heating, Plasma Oscillations, Plasma Turbulence, Plasma Waves, Resistance Heating, Shock Heating, Shock Waves, Transition Points, Data Bases, Earth (Planet)

Scientific paper

A data set containing measurements for approximately 100 shock crossings was compiled, and plasma wave profiles were plotted in conjunction with magnetic field data. Three emissions analyzed include upstream electron plasma oscillations, ion acoustic noise, and low frequency electromagnetic noise. The data demonstrate that the observed waves are consistent with generation by the kinetic cross-field streaming instability. Reanalysis of shock overshoots prompted by the presence of plasma feet upstream of nominally subcritical shocks leads to the conclusion that no firm evidence exists for a sharp subcritical supercritical transition. Electron plasma oscillations persist up to the ramps of subcritical shocks and begin decaying at the front edge of the feet of supercritical shocks. Their intensity is anticorrelated with the amplitude of the foot ion acoustic noise. Wave measurements support the predicted predominance of lower hybrid-like modes over ion acoustic noise in the production of resistive (plasma) heating. Evidence for variable shock normal angles is seen upstream from nominally quasiparallel shocks. The first cases of very strong electron heating observed at the terrestrial bow shock were discovered.

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