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

TL;DR
This paper investigates how suprathermal solar particles, which increase solar wind pressure during high activity, may affect the Earth's magnetosphere's ability to transmit low-energy cosmic rays, based on a recent solar event.
Contribution
It provides an estimation of the impact of suprathermal particles on magnetospheric transmissivity during solar activity, highlighting a potential influence on cosmic ray shielding.
Findings
Suprathermal particles increase solar wind pressure during high activity.
Elevated pressure may alter magnetospheric transmissivity.
Analysis based on a recent solar event.
Abstract
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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Taxonomy
TopicsIonosphere and magnetosphere dynamics · Solar and Space Plasma Dynamics · Earthquake Detection and Analysis
