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Formation of Suprathermal Electron Populations in the Expanding, Turbulent Solar Wind

  • Authors: Maximilien Péters de Bonhome, Fabio Bacchini, Luca Pezzini, Viviane Pierrard

Maximilien Péters de Bonhome et al 2026 The Astrophysical Journal Letters 1005 .

  • Provider: AAS Journals

Caption: Figure 2.

(a) Evolution of the box-averaged magnetic-field strength normalized by the initial background magnetic field. (b) Evolution of the rms speed of electrons (in blue), ions (in red), and the magnetic-field fluctuations normalized by the background magnetic field in black. (c) Evolution of the average temperature ratio, T/T, for electrons (in blue) and ions (in red), with the associated firehose instability thresholds plotted as corresponding dashed lines. The vertical dashed lines indicate the onset of expansion at ﹩{t}_{{\rm{\exp }}}=0.5{\tau }_{{\rm{\exp }}}﹩ and triggering of the electron firehose instability at ﹩{t}_{{\rm{EFI}}}=0.75{\tau }_{{\rm{\exp }}}﹩.

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