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Probing Solar Wind Structures with Solar Energetic Particle Observations from Solar Orbiter

  • Authors: Xiaohang Chen, Gang Li, Joe Giacalone, Xiangliang Kong, Shuai Fu, Rumeng Zhang, Changyue Zhao, George C. Ho, David Lario, Zheyi Ding, Robert F. Wimmer-Schweingruber, Glenn M. Mason, Roberto Bruno, Nicolas Wijsen, Javier Rodríguez-Pacheco, Xianzhi Ao, Bingxian Luo

Xiaohang Chen et al 2026 The Astrophysical Journal Letters 1008 .

  • Provider: AAS Journals

Caption: Figure 3.

SEP and solar wind observations from 05:30 to 10:00 UT on 2023 December 15. The SFD interval is marked by vertical dotted lines. (a)–(d) Background-subtracted energy spectrograms in four looking directions. (e) Magnetic field components in RTN coordinates. (f) Proton number density. (g) Proton temperature. (h) Bulk solar wind speed. (i) The angle between the magnetic field and the ambient solar wind flow. (j) Normalized magnetic field deflection.

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