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Proton Temperature Anisotropy across Interplanetary Shocks: A Statistical Analysis with WIND Observations

  • Authors: Zeping Jin, Lingling Zhao, Xingyu Zhu, Vladimir Florinski, Gary P. Zank, Jakobus Le Roux, Yiming Jiao, Ashok Silwal, Nibuna S. M. Subashchandar

Zeping Jin et al 2026 The Astrophysical Journal Letters 1002 .

  • Provider: AAS Journals

Caption: Figure 4.

Statistical distribution of (T/T, β) upstream and downstream of fast-forward shocks. The black dashed or dotted lines indicate theoretical thresholds for various instabilities with growth rate γ = 10−3 ωcp (dotted: mirror instability; dashed: proton cyclotron instability; dashed–dotted: parallel fire-hose instability; dashed–dotted–dotted: oblique fire-hose instability). The top panels show the 0–1 minute interval immediately near the shock, while the bottom panels show the 1–10 minute interval farther from the shock. These time windows correspond to those used in Figure 3. Red contours represent the density distribution, and its levels span from 10% to 50% of the maximum value with equal spacing.

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