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• W2015595087 abstract "Context. In recent years the accumulation of magnetic helicity via emergence of new magnetic flux and/or shearing photospheric motions has been considered to play an important role in the destabilization processes that lead to eruptive phenomena occurring in the solar atmosphere." @default.
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• W2015595087 date "2010-11-26" @default.
• W2015595087 modified "2023-10-03" @default.
• W2015595087 title "A solar eruption triggered by the interaction between two magnetic flux systems with opposite magnetic helicity" @default.
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• W2015595087 doi "https://doi.org/10.1051/0004-6361/201014437" @default.
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