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The Wave-regulated Precursor of a Near-parallel Interplanetary Shock Observed by Parker Solar Probe

  • Authors: I. C. Jebaraj, L. Colomban, O. V. Agapitov, M. Gedalin, M. A. Malkov, A. Kouloumvakos, E. Husidic, S. Mondal, S. Yadav, N. Wijsen

I. C. Jebaraj et al 2026 The Astrophysical Journal Letters 1008 .

  • Provider: AAS Journals

Caption: Figure 4.

The energetic-particle precursor and the compressive amplitude over 06:00–07:13 UT on 2023 March 13; the time axis corresponds to shock-normal distance through x = u1(tshock − t), and the dashed line marks the shock. (a) Energetic-particle pressure PEP (green) with its exponential fit of scale length LEP ≃ 5.48 R (black dashed). (b) The compressive amplitudes δn/n (maroon) and δB/B0 (black), the in-phase coherent components in the LP-OB band (Appendix C), with the energetic-particle-gradient forced response ﹩{ \mathcal N }/({M}_{f}^{2}-1)﹩ (gray dotted).

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