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• W2891529914 endingPage "155" @default.
• W2891529914 startingPage "155" @default.
• W2891529914 abstract "A fundamental problem in plasma and astrophysics is the motion of energetic and electrically charged particles through a magnetized plasma, e.g., cosmic rays propagating through the interplanetary or interstellar medium. In particular, the motion of particles across a large-scale or guide field is difficult to describe analytically. Recently, an advanced nonlinear theory for perpendicular transport was developed. The theory shows good agreement with simulations and can be used for a variety of synthetic turbulence models. An interesting feature of the latter theory is that it allows for a full time-dependent description of perpendicular transport, including the initial ballistic motion, sub-diffusion, and the recovery of diffusion as soon as there is transverse complexity of the magnetic field. It is the purpose of the current paper to use this theory to derive analytical forms of the time-dependent perpendicular diffusion parameter for different cases. This is useful for a variety of applications, such as studies of shock acceleration and solar modulation." @default.
• W2891529914 created "2018-09-27" @default.
• W2891529914 creator A5089414236 @default.
• W2891529914 date "2018-09-12" @default.
• W2891529914 modified "2023-09-24" @default.
• W2891529914 title "Analytical Description of the Time-dependent Perpendicular Transport of Energetic Particles" @default.
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• W2891529914 doi "https://doi.org/10.3847/1538-4357/aadaeb" @default.
• W2891529914 hasPublicationYear "2018" @default.
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