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

P. Bobik , M. J. Boschini , C. Consolandi , S. Della Torre , M. Gervasi , D. Grandi , K. Kudela , G. La Vacca

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M. Mallamaci S. Pensotti P.G. Rancoita D. Rozza M. Tacconi

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classification 🌌 astro-ph.IM astro-ph.EPastro-ph.SRphysics.space-ph

keywords solarpressuresuprathermalwindcosmicmagnetosphericparticlesrays

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

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

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