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- W4297901860 abstract "Context. A standard model for eruptive flares aims at describing observational 3D features of the reconnecting coronal magnetic field. Extensions to the 2D model require the physical understanding of 3D reconnection processes at the origin of the magnetic configuration evolution. However, the properties of 3D reconnection without null point and separatrices still need to be analyzed." @default.
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- W4297901860 date "2013-07-01" @default.
- W4297901860 modified "2023-10-18" @default.
- W4297901860 title "The standard flare model in three dimensions" @default.
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- W4297901860 doi "https://doi.org/10.1051/0004-6361/201321164" @default.
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