August 1972 solar-terrestrial events - Observations of interplanetary shocks at 2.2 AU

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Interplanetary Medium, Propagation Velocity, Shock Wave Propagation, Solar Activity Effects, Solar Flares, Interplanetary Magnetic Fields, Pioneer 10 Space Probe, Pioneer 9 Space Probe, Solar Wind Velocity

Scientific paper

Simultaneous magnetic field and plasma observations on Pioneer 10 were used to identify three shocks and a plasma driver (possible flare ejecta) at 2.2 AU caused by the four large solar flares of August 2-7, 1972. Two shocks, the first and third, were forward shocks, while the second was a reverse shock. The local inertial velocities of all three shocks were estimated under the assumption of quasi-perpendicularity, i.e., the shocks were assumed to be propagating principally across, rather than along, the interplanetary magnetic field.

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