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Investigating the Effect of IMF Path Length on Pitch-angle Scattering of Strahl within 1 au
Strahl is the strongly field-aligned, beam-like population of electrons in the solar wind. Strahl width is observed to increase with distance from the Sun, and hence strahl electrons must be subject to in-transit scattering effects. Different energy relations have been both observed and modeled for both strahl width and the width increase with radial distance. Thus, there is much debate regarding what mechanism(s) scatter strahl. In this study, we use a novel method to investigate strahl evolution within 1 au by estimatin ...
Graham, G.; Rae, I.; Owen, C.; Walsh, A.;
Published by: The Astrophysical Journal Published on: 03/2018
YEAR: 2018   DOI: 10.3847/1538-4357/aaaf1b
parker solar probe; plasmas; scattering; Solar Probe Plus; Solar wind; Sun: heliosphere