Plasma Heating Induced by Tadpole-like Downflows in the Flaring Solar Corona

As one of the most spectacular energy release events in the solar system, solar flares are generally powered by magnetic reconnection in the solar corona. As a result of the re-arrangement of magnetic field topology after the reconnection process, a series of new loop-like magnetic structures are of...

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Detalles Bibliográficos
Autores principales: Samanta, Tanmoy, Tian, Hui, Chen, Bin, Reeves, Katharine K., Cheung, Mark C.M., Vourlidas, Angelos, Banerjee, Dipankar
Formato: Online Artículo Texto
Lenguaje:English
Publicado: Elsevier 2021
Materias:
Report
Acceso en línea:https://www.ncbi.nlm.nih.gov/pmc/articles/PMC8454670/
https://www.ncbi.nlm.nih.gov/pubmed/34557738
http://dx.doi.org/10.1016/j.xinn.2021.100083

Internet

https://www.ncbi.nlm.nih.gov/pmc/articles/PMC8454670/
https://www.ncbi.nlm.nih.gov/pubmed/34557738
http://dx.doi.org/10.1016/j.xinn.2021.100083

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