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Turbulence and Waves in the Sub-Alfvénic Solar Wind Observed by the Parker Solar Probe during Encounter 10

  • Authors: L.-L. Zhao, G. P. Zank, L. Adhikari, D. Telloni, M. Stevens, J. C. Kasper, S. D. Bale, N. E. Raouafi

L.-L. Zhao et al 2022 The Astrophysical Journal Letters 934 .

  • Provider: AAS Journals

Caption: Figure 4.

MHD wave mode decomposition from 21:00 on November 21 to 10:00 on November 22. The left panels from top to bottom show the Alfvén Mach number M A , the wavelet trace PSD of the magnetic field fluctuations, and the angle between wavevector k and the local mean magnetic field ﹩{\theta }_{{\boldsymbol{k}},{{\boldsymbol{B}}}_{0l}}﹩. The other six panels show the relative fraction of the spectral energy density in each MHD wave mode.

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