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...
Збережено в:
| Автори: | , , , |
|---|---|
| Формат: | Artigo |
| Мова: | Inglês |
| Опубліковано: |
IOP Publishing
2025-01-01
|
| Серія: | The Astrophysical Journal Letters |
| Предмети: | |
| Онлайн доступ: | https://doi.org/10.3847/2041-8213/ad9ddd |
| Теги: |
Немає тегів, Будьте першим, хто поставить тег для цього запису!
|