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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 5.

Same as Figure 3, but for the unsteady loop top at t = 138 s, perturbed by a plasmoid collision. In contrast to the quasi-steady case, the outward plasma flow (d) now aligns with the magnetic field gradient (e), leading to positive betatron acceleration (f). Black boxes mark the selected electron trajectory regions from Figure 4.

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