Jovian S-burst Drift Rates and S-burst/L-burst Interactions in a Phase-bunching Model

Details Jovian S-burst Drift Rates and S-burst/L-burst Interactions in a Phase-bunching Model Jovian S-burst Drift Rates and S-burst/L-burst Interactions in a Phase-bunching Model

Dec 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001agufmsm12a0832w&link_type=abstract

American Geophysical Union, Fall Meeting 2001, abstract #SM12A-0832

Physics

2756 Planetary Magnetospheres (5443, 5737, 6030), 7839 Nonlinear Phenomena, 7847 Radiation Processes, 7867 Wave/Particle Interactions, 7871 Waves And Instabilities

Scientific paper

A nonlinear feedback mechanism for the generation of jovian S-bursts is re-examined in the light of recent observations of phase coherence in jovian S-bursts. In this model, phase-coherent radiation is generated by phase-bunched electrons within interaction regions drifting along the Io flux tube. Evaluation of S-burst drift rates reveals that several unexplained properties of S-bursts, namely, their complex morphologies and interactions with narrowband L-bursts, are consistent with a phase-bunching model.

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