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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 5.

Temperature anisotropies (N/A) for different electron components in each column for different regions and shock parameters (i.e., color-coded labels by row). The top row shows all (violet), upstream (blue), and downstream (red) anisotropies. The middle row shows low Mach number (blue) and high Mach number (red) anisotropies. The bottom row shows quasi-parallel (blue) and quasi-perpendicular (red) anisotropies.

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