Transverse oscillations and an energy source in a strongly magnetized sunspot

The solar corona is two to three orders of magnitude hotter than the underlying photosphere, and the energy loss of coronal plasma is extremely strong, requiring a heating flux of over 1,000 W m(−2) to maintain its high temperature. Using the 1.6 m Goode Solar Telescope, we report a detection of ubi...

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Detalles Bibliográficos
Autores principales: Yuan, Ding, Fu, Libo, Cao, Wenda, Kuźma, Błażej, Geeraerts, Michaël, Trelles Arjona, Juan C., Murawski, Kris, Van Doorsselaere, Tom, Srivastava, Abhishek K., Miao, Yuhu, Feng, Song, Feng, Xueshang, Noda, Carlos Quintero, Cobo, Basilio Ruiz, Su, Jiangtao
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/PMC10356614/
https://www.ncbi.nlm.nih.gov/pubmed/37483848
http://dx.doi.org/10.1038/s41550-023-01973-3

Internet

https://www.ncbi.nlm.nih.gov/pmc/articles/PMC10356614/
https://www.ncbi.nlm.nih.gov/pubmed/37483848
http://dx.doi.org/10.1038/s41550-023-01973-3

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