Coronal Hole Boundary Region: Multiple Facets and Connection to the Slow Solar Wind
It is commonly recognized that a coronal hole (CH) boundary region exists where the slow solar wind (SW) is formed by more than one physical process. The physical properties at the CH boundary region play an important role in dictating the slow SW properties by providing conditions for the relevant...
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| Главные авторы: | , , , , |
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| Формат: | Artigo |
| Язык: | Inglês |
| Опубликовано: |
IOP Publishing
2026-01-01
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| Серии: | The Astrophysical Journal |
| Предметы: | |
| Online-ссылка: | https://doi.org/10.3847/1538-4357/ae32ee |
| Метки: |
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