The influence of transient solar-wind events on the cosmic-ray intensity modulation.

Physics

Scientific paper

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Cosmic Rays: Solar Modulation

Scientific paper

Studies the behavior of cosmic rays, observed by three stations during a time of high-speed solar wind (HSSW) events. These stations cover the median rigidity range 16 - 164 GV. The influence of the interplanetary magnetic field (IMF) associated with HSSW has also been studied. The analysis covers the period 1967 - 1986. Both the cosmic ray intensity and geomagnetic activity are enhanced by coronal mass ejection events. The IMF magnitude and fluctuation are responsible for the depression of cosmic ray intensity during HSSW events.

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