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...

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Detalles Bibliográficos
Autores principales: Schwanitz, Conrad, Harra, Louise, Raouafi, Nour E., Sterling, Alphonse C., Moreno Vacas, Alejandro, del Toro Iniesta, Jose Carlos, Orozco Suárez, David, Hara, Hirohisa
Formato: Online Artículo Texto
Lenguaje:English
Publicado: Springer Netherlands 2021
Materias:
Article
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

Internet

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

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