The upstream region, foreshock and bow shock wave at Halley's Comet from plasma electron measurements

Details The upstream region, foreshock and bow shock wave at Halley's Comet from plasma electron measurements The upstream region, foreshock and bow shock wave at Halley's Comet from plasma electron measurements

Dec 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986esasp.250a.259a&link_type=abstract

In ESA Proceedings of the 20th ESLAB Symposium on the Exploration of Halley's Comet. Volume 1: Plasma and Gas p 259-261 (SEE N87

Physics

Plasma Physics

3

Bow Waves, Electron Density Profiles, Electrons, Plasma Physics, Shock Waves, Space Plasmas, Electron Energy, Flux (Rate), Plasma-Particle Interactions, Solar Wind

Scientific paper

The authors survey the plasma electron parameters from a distance 2.7×106km from the comet nucleus to the bow shock wave at about 1.1×106km and somewhat beyond. They describe the features of the electron foreshock lying outside the shock to a distance of about 230,000 km. It is a region of intense solar wind-comet plasma interaction in which energetic electrons are prominent. Several spikes of electrons whose energies extend to about 2.5 keV appear in front of the shock. These energetic electrons may have been accelerated in the same way electrons are accelerated at the Earth's bow shock to energies of 1 to 10 keV. The direction of the electron bulk flow direction changes abruptly between 1920 and 1922 UT, and the flow speed begins a sharp decline at the same time. The authors believe the spacecraft has entered the bow shock wave sometimes between 1920 and 1922 UT. They find that the electron density variations at Halley are very much smaller than those reported at Giacobini-Zinner.

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