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Potgieter, M.S. and Langner, U.W. (2005) Modulation of Cosmic Rays: Perpendicular Diffusion and Drifts in a Heliosphere with a Solar Wind Termination Shock. Advances in Space Research, 35, 554-561.
https://doi.org/10.1016/j.asr.2005.01.008

has been cited by the following article:

• TITLE: Transport in Astrophysics: VII. Solar Modulation of the Cosmic Rays

  AUTHORS: Lorenzo Zaninetti

  KEYWORDS: Cosmic Rays, Particle Diffusion, Random Walks

  JOURNAL NAME: International Journal of Astronomy and Astrophysics, Vol.14 No.4, November 5, 2024

  ABSTRACT: Two existing solutions for the diffusion of cosmic rays (CRs) are analyzed. The first one is a well-known solution in 3D over an infinite spatial domain and the second one is a 1D solution with an exponential decay initial profile over an infinite spatial domain. For each solution, the temporal evolution of the number of particles at a fixed distance has been analyzed. The anticorrelation between the flux of CRs and the magnetic field at one astronomical unit has been explained by adopting a careful choice of the astrophysical parameters involved.