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Electron Energy Partition across Interplanetary Shocks. II. Statistics

  • Authors: Lynn B. Wilson, Li-Jen Chen, Shan Wang, Steven J. Schwartz, Drew L. Turner, Michael L. Stevens, Justin C. Kasper, Adnane Osmane, Damiano Caprioli, Stuart D. Bale, Marc P. Pulupa, Chadi S. Salem, and Katherine A. Goodrich

2019 The Astrophysical Journal Supplement Series 245 24.

  • Provider: AAS Journals

Caption: Figure 2.

Densities (cm−3) and density ratios for different ion and electron components as a percentage of the total number of finite points (i.e., color-coded numbers in each panel). The format is similar to Figure 1 with the row organization, but the columns differ. The first column here shows proton (violet) and alpha-particle (blue) density from Wind/SWE and total ion density from Wind/3DP (red). The second column shows nes for the core (violet), halo (blue), and beam/strahl (red) components. The third column shows ﹩{n}_{s}/{n}_{s^{\prime} }﹩ for the halo-to-core (violet), beam-to-core (blue), and beam-to-halo (red) density ratios. The corresponding one-variable statistics for the electron parameters are shown in Table 3. Note that the nα, neh, neb, and all three ﹩{n}_{s}/{n}_{s^{\prime} }﹩ values were offset by constant factors (shown in panels (a), (d), and (g)) to reduce the horizontal axis dynamic range.

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