2020
DOI: 10.1002/ctpp.202000164
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Numerical study of penetration and distribution of charged particles in the magnetosphere during southward IMF case

Abstract: The energetic charged particles penetration in the plasmasphere are carried out using the updated version of 3D Stanford PIC code. We considered slow and fast wind streams to know the penetration of the energetic charged particles (electrons and ions) having different velocities into four regions i.e. cusp, plasmasphere, sunward, and tailward sides. It is observed that the ion penetrations are higher than electrons for solar slow wind streams in the plasmasphere, while it is reverse for the solar fast streams.… Show more

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“…In this paper, we adopt the same simulation model with dimensions (x=215, y=145, z=145) that has previously been used by Esmaeili & Kalaee [2017] and Esmaeili et al [2020]. In the simulation, 1 equals to 0.5 R E where 1 R E is approximately 6400 km.…”
Section: -1 Initial Parametersmentioning
confidence: 99%
“…In this paper, we adopt the same simulation model with dimensions (x=215, y=145, z=145) that has previously been used by Esmaeili & Kalaee [2017] and Esmaeili et al [2020]. In the simulation, 1 equals to 0.5 R E where 1 R E is approximately 6400 km.…”
Section: -1 Initial Parametersmentioning
confidence: 99%