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• W2580456983 abstract "Significance Electron two-stream instability (ETSI) is believed to be responsible for the radio bursts observed in both the solar corona and interplanetary medium. What nonlinear kinetic processes self-consistently reconcile the several orders of magnitude difference between the short linear saturation time scale of ETSI and the long duration of bursts is fundamental in plasma turbulence and has remained unsolved for nearly 50 y. Using massive particle-in-cell simulations, we find a self-consistent and complete nonlinear solution to this problem." @default.
• W2580456983 created "2017-02-03" @default.
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• W2580456983 date "2017-01-30" @default.
• W2580456983 modified "2023-10-07" @default.
• W2580456983 title "How electron two-stream instability drives cyclic Langmuir collapse and continuous coherent emission" @default.
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• W2580456983 doi "https://doi.org/10.1073/pnas.1614055114" @default.
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