Physics
Scientific paper
Aug 1982
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982georl...9..881p&link_type=abstract
Geophysical Research Letters, vol. 9, Aug. 1982, p. 881-884. Research sponsored by the U.S. Department of Energy
Physics
111
Bow Waves, Shock Wave Interaction, Solar Terrestrial Interactions, Solar Wind, Space Plasmas, Gyration, International Sun Earth Explorer 1, Ion Beams, Velocity Distribution
Scientific paper
A beam of secondary ions which gyrate about the magnetic field have been detected by ISEE-1 satellite measurements of ion velocity distributions during a high Mach number bow shock crossing under nearly perpendicular conditions. The ions are encountered as the satellite enters the region ahead of the foot of the shock, and their behavior is that of solar wind ions reflected off the shock and then returned to it under the combined influence of magnetic field deflection and interplanetary electric field acceleration. Beam densities increase from 0.2 to 30% of the total plasma density as the main shock is approached, and the ion beam is not degraded through interaction with the counterstreaming solar wind upstream of the ramp. The gyrating ions provide strong dispersion in velocity space, and therefore constitute the first step in the process by which solar wind streaming energy is converted into the thermal energy of the ions at the bow shock.
Bame J. Jr. S.
Gosling Jack T.
Paschmann Goetz
Sckopke Norbert
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