Electron acceleration by wave turbulence in a magnetized plasma
Astrophysical shocks are commonly revealed by the non-thermal emission of energetic electrons accelerated in situ1,2,3. Strong shocks are expected to accelerate particles to very high energies4,5,6; however, they require a source of particles with velocities fast enough to permit multiple shock cros...
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| Materialtyp: | Journal article |
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Springer Nature
2018
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