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Energetic (suprathermal) solar particles, accelerated in the interplanetarymedium, contribute to the solar wind pressure, in particular during high solaractivity periods. We estimated the effect of the increase of solar windpressure due to suprathermal particles on magnetospheric transmissivity ofgalactic cosmic rays in the case of one recent solar event.

Suprathermal particle addition to solar wind pressure: possible influence on magnetospheric transmissivity of low energy cosmic rays?