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Alpha–Proton Relative Drift: Implications for the Origins and Dynamics of the Solar Wind

Helium nuclei (alpha particles) strongly influence the momentum and energy balance in the solar wind, comprising up to 20% of the solar wind mass density. In fast Alfvénic wind at heliocentric distances greater than 0.3 au, the alpha particles’ bulk flow speed is systematically different to that of...

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Detalles Bibliográficos
Principais autores: Joseph H. Wang, Timothy S. Horbury, Lorenzo Matteini, Domenico Trotta
Formato: Artigo
Idioma:Inglês
Publicado: IOP Publishing 2025-01-01
Series:The Astrophysical Journal Letters
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Acceso en liña:https://doi.org/10.3847/2041-8213/ad9ddd
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