Bercic, Laura; Larson, Davin; Whittlesey, Phyllis; Maksimovic, Milan; Badman, Samuel T.; Landi, Simone; Matteini, Lorenzo; Bale, Stuart D.; Bonnell, John W.; Case, Anthony W.; Dudok de Wit, Thierry; Goetz, Keith; Harvey, Peter R.; Kasper, Justin C.; Korreck, Kelly E.; Livi, Roberto; MacDowall, Robert J.; Malaspina, David M.; Pulupa, Marc; Stevens, Michael L.
(2020)
The shape of the electron velocity distribution function plays an important role in the dynamics of the solar wind acceleration. Electrons are normally modeled with three components, the core, the halo, and the strahl. We ...