Magnetic field line transport in the heliosphere and energetic particle propagation from corotating interaction regions to high heliographic latitudes

DOI10.1023/A:1012223925955zbMath0989.85005OpenAlexW1558214240MaRDI QIDQ5952683

Gaetano Zimbardo, Pierre Pommois, Pierluigi Veltri

Publication date: 1 August 2002

Published in: Astrophysics and Space Science (Search for Journal in Brave)

Full work available at URL: https://doi.org/10.1023/a:1012223925955

zbMATH Keywords

Monte Carlo simulationanisotropysolar windcorotating interaction regionsdiffusion coefficientsmagnetic turbulence

Mathematics Subject Classification ID

Hydrodynamic and hydromagnetic problems in astronomy and astrophysics (85A30)

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