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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 B1.

Wavenumber content of the four upstream wave families, RH, LH, LP-OB, and LP-FA (columns 1–4). Each panel is a ﹩{B}_{w}^{2}﹩-weighted two-dimensional histogram of spacecraft-frame frequency f against the wavenumber k = 2πf/Vφ. White curves are the plasma-frame branches (R-mode, L-mode, fast magnetosonic at the LP-OB median θkB, and shear Alfvén), Doppler shifted into the spacecraft frame.

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