Three dimensional propagation characteristics of the flare-associated interplanetary shockwave during 1978-1981

Computer Science – Sound

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Interplanetary Medium, Satellite Sounding, Shock Wave Propagation, Solar Activity Effects, Solar Flares, Interplanetary Magnetic Fields, Scientific Satellites

Scientific paper

Japanese IPS flare data obtained during years of high solar activity (1978-1981) are used to study the three-dimensional propagation characteristics of the flare-associated shock wave. Particular attention is given to the dynamic effects of shock-wave propagation. The results show that: (1) the propagation of the shock wave is asymmetrical relative to the normal direction of the flare; (2) the propagating range of the latitudes is less than that of the longitudes; and (3) there are sharp east-west and north-south asymmetries in the shock wave energy distribution which determine the anisotropies of shock wave propagation. The results suggest both magnetic structures near the sun and interplanetary large-scale solar wind structures have significant modulating effects on the three-dimensional propagation of the shock wave.

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