Interplanetary flow systems associated with cosmic ray modulation in 1977-1980

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Galactic Cosmic Rays, Interplanetary Magnetic Fields, Magnetohydrodynamic Flow, Solar Cycles, Solar Wind, Energetic Particles, Helios 1, Modulation, Shock Waves, Voyager 1 Spacecraft, Voyager 2 Spacecraft

Scientific paper

The hydromagnetic flow configurations associated with the cosmic ray modulation in 1977 - 1980 were determined using solar wind plasma and magnetic field data from Voyager 1 and 2 and Helios 1. The modulation was related to two types of large-scale systems of flows: one containing a number of transients such as shocks and postshock flows, the other consisting primarily of a series of quasi-stationary flows following interaction regions containing a stream interface and often bounded by a forward-reverse shock pair. Each of three major episodes of cosmic ray modulation was associated with the passage of a system of transient flows. Plateaus in the cosmic ray intensity-time profile were associated with the passage of systems of corotating streams.

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