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Reconnection-induced Electron Energization in Magnetospheric Kelvin–Helmholtz Dynamics

  • Authors: Silvia Ferro, Fabio Bacchini, Giuseppe Arrò, Francesco Pucci, Pierre Henri

Silvia Ferro et al 2026 The Astrophysical Journal Letters 1008 .

  • Provider: AAS Journals

Caption: Figure 3.

Temporal evolution of the energy transfer channels during the nonlinear stage of the KHI. Panels (a) and (b) show the spatially averaged parallel and perpendicular components of the electromagnetic work, ﹩\left\langle {J}_{\parallel }{E}_{\parallel }\right\rangle ﹩ and 〈JE〉, respectively, for electrons (blue) and ions (red), separately in the LS (solid lines) and US (dashed lines). Panels (c) and (d) show the time-integrated cumulative contributions for electrons and ions, respectively: ∫J  ·  E dt, ∫Π: D dt, and ∫ dt, normalized to the initial total energy Etot,0.

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