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pro vyhledávání: '"Gabriele Cozzo"'
Publikováno v:
Symmetry, Vol 15, Iss 3, p 627 (2023)
The bright solar corona entirely consists of closed magnetic loops rooted in the photosphere. Photospheric motions are important drivers of magnetic stressing, which eventually leads to energy release into heat. These motions are chaotic and obviousl
Externí odkaz:
https://doaj.org/article/4e9b8c35fe7b4052b2f73da734797a29