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• W1972580894 abstract "<i>Context. <i/>We investigate the nonlinear evolution of the electron distribution in the presence of the strong inductive electric field in the reconnecting current sheets (RCS) of solar flares.<i>Aims. <i/>We aim to study the characteristics of nonthermal electron-beam plasma instability and its influence on electron acceleration in RCS.<i>Methods. <i/>Including the external inductive field, the one-dimensional Vlasov simulation is performed with a realistic mass ratio for the first time.<i>Results. <i/> Our principal findings are as follows: 1) the Buneman instability can be quickly excited on the timescale of 10<sup>-7<sup/> s for the typical parameters of solar flares. After saturation, the beam-plasma instabilities are excited due to the non-Maxwellian electron distribution; 2) the final velocity of the electrons trapped by these waves is of the same order as the phase speed of the waves, while the untrapped electrons continue to be accelerated; 3) the inferred anomalous resistance of the current sheet and the energy conversion rate are basically of the same order as those previously estimated, e.g., “the analysis of Martens”.<i>Conclusions. <i/>The Buneman instability is excited on the timescale of 10<sup>-7<sup/> s and the wave-particle resonant interaction limits the low-energy electrons to be further accelerated in RCS." @default.
• W1972580894 created "2016-06-24" @default.
• W1972580894 creator A5012237055 @default.
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• W1972580894 date "2009-06-04" @default.
• W1972580894 modified "2023-10-16" @default.
• W1972580894 title "Electron acceleration in the turbulent reconnecting current sheets in solar flares" @default.
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• W1972580894 doi "https://doi.org/10.1051/0004-6361/200811494" @default.
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