VLF emissions in the Venus foreshock - Comparison with terrestrial observations

Details VLF emissions in the Venus foreshock - Comparison with terrestrial observations VLF emissions in the Venus foreshock - Comparison with terrestrial observations

Sep 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993jgr....9815305c&link_type=abstract

Journal of Geophysical Research (ISSN 0148-0227), vol. 98, no. A9, p. 15,305-15,317.

Physics

8

Bow Waves, Interstellar Magnetic Fields, Shock Waves, Solar Wind, Venus (Planet), Electron Plasma, Emission Spectra, Ion Acoustic Waves, Solar Planetary Interactions, Very Low Frequencies

Scientific paper

An examination is conducted of ELF/VLF emissions observed in the solar wind upstream of the Venus shock, for the 100 Hz-30 kHz range, using data from the Pioneer Venus Orbiter's electric field detector and magnetometer instruments. Detailed comparisons are made with terrestrial measurements for both the electron and ion foreshocks. The results obtained support the Crawford et al. (1990) identification of the Venus electron foreshock emissions as electron plasma oscillations, whose waves are generated in situ and act to isotropize the electron distributions.

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