Electron–Ion Heating Partition in Imbalanced Solar-wind Turbulence
A likely candidate mechanism to heat the solar corona and solar wind is low-frequency “Alfvénic” turbulence sourced by magnetic fluctuations near the solar surface. Depending on its properties, such turbulence can heat different species via different mechanisms, and the comparison of theoretical pre...
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| Principais autores: | , , |
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| Formato: | Artigo |
| Idioma: | Inglês |
| Publicado em: |
IOP Publishing
2023-01-01
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| coleção: | The Astrophysical Journal Letters |
| Assuntos: | |
| Acesso em linha: | https://doi.org/10.3847/2041-8213/ad0779 |
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