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Wave Composition, Propagation, and Polarization of Magnetohydrodynamic Turbulence within 0.3 au as Observed by Parker Solar Probe

  • Authors: Xingyu Zhu, Jiansen He, Daniel Verscharen, Die Duan, and Stuart D. Bale

2020 The Astrophysical Journal Letters 901 L3.

  • Provider: AAS Journals

Caption: Figure 1.

Time sequences overview of magnetic and plasma measurements during PSP’s first encounter. Panel (a): magnetic field strength (﹩| B| ﹩) and proton density (Np). Panels (b), (c), and (d): magnetic fields (﹩{B}_{{\rm{R}}},{B}_{{\rm{T}}},{B}_{{\rm{N}}}﹩) and proton bulk velocities (﹩{V}_{{\rm{R}},{\rm{p}}},{V}_{{\rm{T}},{\rm{p}}},{V}_{{\rm{N}},{\rm{p}}}﹩) in RTN coordinates. Panel (e): proton density (Np) and thermal velocity (Wp). Panel (f): plasma beta (β) and heliocentric distance (R) of spacecraft’s position.

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