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• W3103302510 abstract "Context. In solar flares, a large number of charged particles is accelerated to high energies. By which physical processes this is achieved is one of the main open problems in solar physics. It has been suggested that during a flare, regions of the rapidly relaxing magnetic field can form a collapsing magnetic trap (CMT) and that this trap may contribute to particle energisation." @default.
• W3103302510 created "2020-11-23" @default.
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• W3103302510 date "2014-07-01" @default.
• W3103302510 modified "2023-09-23" @default.
• W3103302510 title "Particle energisation in a collapsing magnetic trap model: the relativistic regime" @default.
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• W3103302510 doi "https://doi.org/10.1051/0004-6361/201423886" @default.
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