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Electron Velocity Moments in the Solar Wind. II. Statistical Properties

  • Authors: Lynn B. Wilson, Stuart D. Bale, Michael L. Stevens, Bennett A. Maruca, Kristopher G. Klein, Mihailo M. Martinović, Jason M. TenBarge

Lynn B. Wilson et al 2026 The Astrophysical Journal 1002 .

  • Provider: AAS Journals

Caption: Figure 1.

Calibrated electron velocity moments shown as 2D column-normalized histograms vs. the solar wind speed, ∣Vop∣. The panels are as follows: (a) ne,int [cm−3]; (b) Te,tot [eV]; (c) Te,∥ [eV]; (d) Te,⊥ [eV]; (e) Ae [N/A]; and (f) ∣qe,∥∣ [μW m−2]. The figure demonstrates the consistency with the results shown in Figure 8 of C. S. Salem et al. (2023). Panel (e) shows a solid black line at unity for convenience (see Appendix A for symbol definitions). Figure 6 in Appendix B provides a proper statistical reference.

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