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- W3098865567 abstract "Cosmic ray propagation is diffusive because of pitch angle scattering by waves. We demonstrate that if the high-amplitude magnetohydrodynamic turbulence with $tilde B/langle Brangle sim 1$ is present on top of the mean field gradient, the diffusion becomes asymmetric. As an example, we consider the vertical transport of cosmic rays in our Galaxy propagating away from a point-like source. We solve this diffusion problem analytically using a one-dimensional Markov chain analysis. We obtained that the cosmic ray density markedly differs from the standard diffusion prediction and has a sizable effect on their distribution throughout the galaxy. The equation for the continuous limit is also derived, which shows limitations of the convection-diffusion equation." @default.
- W3098865567 created "2020-11-23" @default.
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- W3098865567 date "2015-08-26" @default.
- W3098865567 modified "2023-10-13" @default.
- W3098865567 title "Asymmetric diffusion of cosmic rays" @default.
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- W3098865567 doi "https://doi.org/10.1063/1.4928942" @default.
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