2006
DOI: 10.1051/0004-6361:20065237
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Propagation of energetic electrons through the solar corona and the interplanetary medium

Abstract: Aims. The electron transport is investigated numerically after an electron transport model is deduced. Methods. This model for electron propagation considers global electric and magnetic fields, as well as local Coulomb collisions. A new way to handle the electron's pitch angle evolution by using a binary dice within the treatment of the Coulomb scattering is introduced. The conditions in the solar plasma are represented by average and commonly used models, such that numerical simulations can be performed easi… Show more

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