Figure 5 from Wave Composition, Propagation, and Polarization of Magnetohydrodynamic Turbulence within 0.3 au as Observed by Parker Solar Probe

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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 5.

Panel (a): the distance profiles of the ratio between the middle and maximum singular values of the magnetic spectral matrix (λ_mid/λ_max) for the magnetic fluctuations at different periods from 10 to 1000 s. Panel (b): the variations of λ_mid/λ_max with period for the magnetic fluctuations at different distances from 0.17 to 0.24 au.

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