The modulation of cosmic-ray electrons, positrons and helium nuclei as predicted by a drift model with a simulated wavy neutral sheet

Astronomy and Astrophysics – Astrophysics

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Alpha Particles, Neutral Sheets, Positrons, Solar Activity, Solar Cosmic Rays, Solar Electrons, Astronomical Models, Heliosphere, Interplanetary Magnetic Fields

Scientific paper

A recently developed axially-symmetric drift model with a simulated wavy neutral sheet is applied to the modulation of cosmic-ray electrons, positrons, and helium nuclei in the heliosphere. This model can be used to predict the magnitude of charge-dependent modulation. It is found that, at 800 MV, the ratio He/e(-) is strongly dependent on the waviness of the heliospheric neutral sheet for both positive and negative polarity configurations of the interplanetary magnetic field.

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