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Probing Upflowing Regions in the Quiet Sun and Coronal Holes
Recent observations from Parker Solar Probe have revealed that the solar wind has a highly variable structure. How this complex behaviour is formed in the solar corona is not yet known, since it requires omnipresent fluctuations, which constantly emit material to feed the wind. In this article we an...
| Autores principales: | , , , , , , , |
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| Formato: | Online Artículo Texto |
| Lenguaje: | English |
| Publicado: |
Springer Netherlands
2021
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| Materias: | |
| Acceso en línea: | https://www.ncbi.nlm.nih.gov/pmc/articles/PMC8636441/ https://www.ncbi.nlm.nih.gov/pubmed/34866662 http://dx.doi.org/10.1007/s11207-021-01915-0 |