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Numerical Investigation of Efficient Electron Acceleration at an Unsteady Solar Flare Loop Top

  • Authors: Yoshiaki Sato, Takafumi Kaneko, Noriyuki Narukage, Shinsuke Takasao

Yoshiaki Sato et al 2026 The Astrophysical Journal 1006 .

  • Provider: AAS Journals

Caption: Figure 4.

Electron acceleration in the unsteady loop top at t = 138 s, perturbed by a plasmoid collision. The panel layout is the same as in Figure 2. In sharp contrast to the quasi-steady case, both Fermi reflection (orange) and betatron (green) gains are positive. This synergy drives efficient net acceleration, shown by the rapid increase in total kinetic energy (black).

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