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- W2313479056 abstract "Context. Theoretical models and spacecraft observations of solar flares highlight the role of wave-particle interaction for non-local electron acceleration. In one scenario, the acceleration of a large electron population up to high energies is due to the transport of electromagnetic energy from the loop-top region down to the footpoints, which is then followed by the energy being released in dense plasma in the lower atmosphere." @default.
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- W2313479056 date "2016-04-20" @default.
- W2313479056 modified "2023-10-16" @default.
- W2313479056 title "Electron trapping and acceleration by kinetic Alfvén waves in solar flares" @default.
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- W2313479056 doi "https://doi.org/10.1051/0004-6361/201527617" @default.
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