Figure 1 from Electron Energy Partition across Interplanetary Shocks. II. Statistics

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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 1.

Temperatures (eV) for different electron components in each column and for the different regions (i.e., rows) listed in Table 2. In each panel, there are three color-coded histograms for the different field-aligned components defined as follows: total (red), parallel (violet), and perpendicular (blue). All histograms are normalized to the total number of finite points (i.e., black number in each panel) per parameter per component shown as a percentage.

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