A Numerical Study of the effects of a Corotating Interaction Region on cosmic proton and helium transport

Abstract

A Corotating Interaction Region (CIR) is formed when the fast solar wind catches up with the slow solar wind. It is known that the intensity of Galactic Cosmic Rays (GCRs) is modulated by CIRs with the GCR intensity suppressed inside the CIR. Previous numerical studies were mainly confined to GCR protons. For this study we utilize a hybrid GCR transport model which incorporates a Magnetohydrodynamic (MHD) simulated solar wind plasma background with a CIR structure. Additionally, adopting appropriate mass, charge and local interstellar spectra, the hybrid transport model is applied to GCR protons and the two helium isotopes. It is found that both proton and total helium studied at 0.3 GV are modulated by the CIR with their fluxes being depressed. However, the modulation for protons and helium is different with helio-longitude, and interestingly the ratio of the proton to helium flux varies with longitude. Similar results are found for the way in which the two helium isotopic fluxes vary.

A Numerical Study of the Effects of a Corotating Interaction Region on Cosmic-Ray Transport : Some features of different Cosmic-Ray Composition and Rigidity

“…We still utilize the MHD simulated plasma profile for Carrington Rotation 2066 (Jan. 2008), which corresponds to a solar mimimum phase of solar cycle 23. The details of the MHD model and the plasma profile have already been reported previous [5,6].…”