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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 1.

Volume rendering of the z-component of the magnetic-field fluctuations, δBz/Bg, shown at the initial expansion time (﹩t=0.5{\tau }_{{\rm{\exp }}}﹩), mid-expansion time (﹩t=1.0{\tau }_{{\rm{\exp }}}﹩), and final expansion time (﹩t=1.5{\tau }_{{\rm{\exp }}}﹩).

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