Image Details

Choose export citation format:

Preferential Heating of Protons over Alpha Particles near Turbulent Coherent Structures: Parker Solar Probe Observations

  • Authors: Jiayang Xi, Tieyan Wang, Daniel Verscharen, Yan Yang, Luca Sorriso-Valvo, Xinyi Wang, Wenhao Chen, Zuzheng Chen, Zeren Zhima, Chao Xiao, Xiangcheng Dong, Jin Liu, Xiang Li, Guoqi Liu, Naifei Gou, Xiaoxiao Qin, Malcolm Dunlop, Jinbin Cao

Jiayang Xi et al 2026 The Astrophysical Journal Letters 1007 .

  • Provider: AAS Journals

Caption: Figure 2.

Conditional median of the normalized temperature variations for protons (top row) and alpha particles (bottom row) under different PVI thresholds as defined by Equation (2). The different colored curves represent the results for five PVI threshold bins (2 ≤ PVI < 3, 3 ≤ PVI < 4, 4 ≤ PVI < 5, 5 ≤ PVI < 6, and PVI > 6). Panels (a)–(d) show results for the total (﹩\widetilde{{T}_{p}}﹩), parallel (﹩\widetilde{{T}_{p,\parallel }}﹩), and perpendicular (﹩\widetilde{{T}_{p,\perp }}﹩) temperature changes of protons, and panels (d)–(f) show the ﹩\widetilde{{T}_{\alpha }}﹩, ﹩\widetilde{{T}_{\alpha ,\parallel }}﹩, and ﹩\widetilde{{T}_{\alpha ,\perp }}﹩ for alphas.

Other Images in This Article
Copyright and Terms & Conditions

Additional terms of reuse