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Plasma Heating and Energization in Hot-onset Flare Precursor Events

  • Authors: H. Da, J. F. Drake, M. Swisdak

H. Da et al 2026 The Astrophysical Journal Letters 1009 .

  • Provider: AAS Journals

Caption: Figure 5.

(a) The electron and proton distribution function versus energy. The initial spectrum (blue) for the electron and proton are the same as they share the same temperature. Solid curves are the electron spectrum and dashed curves are the proton spectrum at t/τA = 9.5, 13.5, and 17. (b) The locations of electrons with energy exceeding 1.0 ﹩{m}_{i}{C}_{{\rm{A}}}^{2}﹩ and protons with energy exceeding 10.0 ﹩{m}_{i}{C}_{{\rm{A}}}^{2}﹩.

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