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Dash, S., Nandy, D. and Usoskin, I. (2023) Long-Term Forcing of the Sun’s Coronal Field, Open Flux, and Cosmic Ray Modulation Potential during Grand Minima, Maxima, and Regular Activity Phases by the Solar Dynamo Mechanism. Monthly Notices of the Royal Astronomical Society, 525, 4801-4814.
https://doi.org/10.1093/mnras/stad1807

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.