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• W2568061760 abstract "Context. Heating the solar corona requires dissipation of stored magnetic energy, which may occur in twisted magnetic fields. Recently published numerical simulations show that the ideal kink instability in a twisted magnetic thread may trigger energy release in stable twisted neighbours, and demonstrate an avalanche of heating events." @default.
• W2568061760 created "2017-01-13" @default.
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• W2568061760 date "2017-03-17" @default.
• W2568061760 modified "2023-09-27" @default.
• W2568061760 title "A relaxation model of coronal heating in multiple interacting flux ropes" @default.
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• W2568061760 doi "https://doi.org/10.1051/0004-6361/201629589" @default.
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