5 citations · 5 across the 3 of their papers we have counts for
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astro-ph.SR2026
Turbulent Diffusion of Magnetic Field Lines in the Heliosphere
J. V. A. Joubert, R. D. Strauss, J. Light +2
Due to solar wind turbulence, Parker spirals are stochastic. The dispersion of magnetic field lines is described by a convection-diffusion equation for the field line density distr…
astro-ph.SR2024★ 5 cited
Modeling the astrosphere of LHS~1140
K. Scherer, K. Herbst, N. E. Engelbrecht +3
The cosmic ray (CR) flux, as well as the hydrogen flux into the atmosphere of an exoplanet, can change the composition of the atmosphere. Here, we present the CR and hydrogen flux…