A new theory for perpendicular transport of cosmic rays

DOI10.1051/0004-6361:20077260zbMath1139.85004OpenAlexW1976026990WikidataQ68855182 ScholiaQ68855182MaRDI QIDQ5427352

A. Shalchi, Ioannis Kourakis

Publication date: 20 November 2007

Published in: Astronomy & Astrophysics (Search for Journal in Brave)

Full work available at URL: https://doi.org/10.1051/0004-6361:20077260

zbMATH Keywords

diffusionscatteringturbulencecosmic rays

Mathematics Subject Classification ID

Transport processes in time-dependent statistical mechanics (82C70) Statistical mechanics of plasmas (82D10) Hydrodynamic and hydromagnetic problems in astronomy and astrophysics (85A30)

Related Items (5)

Compound perpendicular transport of charged particles with drift, advection, wave propagation effects, and an arbitrary turbulence spectrum ⋮ Random walk of magnetic field lines: analytical theory versus simulations ⋮ Compound diffusion of energetic particles: a Kappa model for the parallel distribution function ⋮ An analytical study of fractional Klein-Kramers approximations for describing anomalous diffusion of energetic particles ⋮ Analytical forms of correlation functions and length scales of astrophysical turbulence

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