Interchange reconnection as the source of the fast solar wind within coronal holes

The fast solar wind that fills the heliosphere originates from deep within regions of open magnetic field on the Sun called ‘coronal holes’. The energy source responsible for accelerating the plasma is widely debated; however, there is evidence that it is ultimately magnetic in nature, with candidat...

Descripción completa

Detalles Bibliográficos
Autores principales: Bale, S. D., Drake, J. F., McManus, M. D., Desai, M. I., Badman, S. T., Larson, D. E., Swisdak, M., Horbury, T. S., Raouafi, N. E., Phan, T., Velli, M., McComas, D. J., Cohen, C. M. S., Mitchell, D., Panasenco, O., Kasper, J. C.
Formato: Online Artículo Texto
Lenguaje:English
Publicado: Nature Publishing Group UK 2023
Materias:
Article
Acceso en línea:https://www.ncbi.nlm.nih.gov/pmc/articles/PMC10247371/
https://www.ncbi.nlm.nih.gov/pubmed/37286648
http://dx.doi.org/10.1038/s41586-023-05955-3

Internet

https://www.ncbi.nlm.nih.gov/pmc/articles/PMC10247371/
https://www.ncbi.nlm.nih.gov/pubmed/37286648
http://dx.doi.org/10.1038/s41586-023-05955-3

Ejemplares similares