Energies of backstreaming protons in the foreshock

Details Energies of backstreaming protons in the foreshock Energies of backstreaming protons in the foreshock

May 1976

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1976stin...7634104g&link_type=abstract

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Physics

Cislunar Space, Solar Protons, Solar Wind, Bow Waves, Particle Trajectories, Proton Energy, Shock Waves

Scientific paper

A predicted pattern of energy vs detector location in the cislunar region is displayed for protons of zero pitch angle traveling upstream away from the quasi-parallel bow shock. The pattern is implied by upstream wave boundary properties. In the solar ecliptic, protons are estimated to have a minimum of 1.1 times the solar wind bulk energy ESW when the wave boundary is in the early morning sector and a maximum of 8.2 ESW when the boundary is near the predawn flank.

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