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arxiv: astro-ph/9808103 · v1 · submitted 1998-08-11 · 🌌 astro-ph

Charged-Particle Motion in Electromagnetic Fields Having at Least One Ignorable Spatial Coordinate

classification 🌌 astro-ph
keywords coordinateelectromagneticfieldignorableleastspatialtheoremacceleration
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We give a rigorous derivation of a theorem showing that charged particles in an arbitrary electromagnetic field with at least one ignorable spatial coordinate remain forever tied to a given magnetic-field line. Such a situation contrasts the significant motions normal to the magnetic field that are expected in most real three-dimensional systems. It is pointed out that, while the significance of the theorem has not been widely appreciated, it has important consequences for a number of problems and is of particular relevance for the acceleration of cosmic rays by shocks.

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  1. Polarized 3D Synthetic Turbulence I: Magnetic Field Line Random Walk

    astro-ph.HE 2026-05 unverdicted novelty 7.0

    Magnetosonic polarization in synthetic turbulence produces field-line diffusion scaling as (δB/B)^4 with subdiffusion matching MHD simulations, unlike the (δB/B)^2 scaling for random polarization.