Ultra-high-resolution observations of persistent null-point reconnection in the solar corona

Magnetic reconnection is a key mechanism involved in solar eruptions and is also a prime possibility to heat the low corona to millions of degrees. Here, we present ultra-high-resolution extreme ultraviolet observations of persistent null-point reconnection in the corona at a scale of about 390 km o...

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Detalles Bibliográficos
Autores principales: Cheng, X., Priest, E. R., Li, H. T., Chen, J., Aulanier, G., Chitta, L. P., Wang, Y. L., Peter, H., Zhu, X. S., Xing, C., Ding, M. D., Solanki, S. K., Berghmans, D., Teriaca, L., Aznar Cuadrado, R., Zhukov, A. N., Guo, Y., Long, D., Harra, L., Smith, P. J., Rodriguez, L., Verbeeck, C., Barczynski, K., Parenti, S.
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/PMC10102217/
https://www.ncbi.nlm.nih.gov/pubmed/37055427
http://dx.doi.org/10.1038/s41467-023-37888-w

Internet

https://www.ncbi.nlm.nih.gov/pmc/articles/PMC10102217/
https://www.ncbi.nlm.nih.gov/pubmed/37055427
http://dx.doi.org/10.1038/s41467-023-37888-w

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