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Reconnection-induced Electron Energization in Magnetospheric Kelvin–Helmholtz Dynamics
Silvia Ferro et al 2026 The Astrophysical Journal Letters 1008 .
Caption: Figure 2.
Temporal evolution of the difference in each domain-integrated energy component during the nonlinear KH stage, normalized to the initial total energy.
© 2026. The Author(s). Published by the American Astronomical Society.
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