Plasma wave turbulence associated with an interplanetary shock

Details Plasma wave turbulence associated with an interplanetary shock Plasma wave turbulence associated with an interplanetary shock

Feb 1979

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1979jgr....84..541g&link_type=abstract

Journal of Geophysical Research, vol. 84, Feb. 1, 1979, p. 541-552. Research supported by the Bundesministerium für Forschung u

Physics

15

Magnetohydrodynamic Flow, Plasma Turbulence, Plasma Waves, Shock Waves, Solar Wind, Electric Fields, Electron Plasma, Electrostatic Waves, Helios 1, Helios 2, Ion Acoustic Waves, Magnetic Fields, Satellite Observation, Whistlers

Scientific paper

The present paper deals with interplanetary shocks, detected and analyzed to date, from the Helios 1 and 2 spacecraft in eccentric solar orbits. The plasma wave turbulence associated with the shock observed on March 30, 1976 is studied in detail. This event is of particular interest because it represents a clearly defined burst of turbulence against a quiet solar wind background both upstream and downstream of the shock. The shock itself is an oblique shock with upstream parameters characterized by a low Mach number, a low beta, and an abnormally large electron to ion temperature ratio. The types of plasma wave detected are discussed.

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