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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 2.

Similar to Figure 1, this figure shows various electron parameters vs. the solar wind speed, ∣Vop∣. The panels are as follows: (a) βe,tot [N/A]; (b) ﹩\frac{{f}_{{\rm{pe}}}}{{f}_{{\rm{ce}}}}﹩ [N/A]; (c) νee [# day−1]; (d) Kn,ee [N/A]; (e) ﹩\frac{{T}_{e,{\rm{tot}}}}{{T}_{p,{\rm{tot}}}}﹩ [N/A]; and (f) ﹩\frac{{\lambda }_{e}}{{\lambda }_{{\rm{De}}}}﹩ [N/A]. Panels (a) and (e) show 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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