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On the applicability of Taylor’s hypothesis in streaming magnetohydrodynamic turbulence

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Figure

Fig. 1 Time series plots of the magnetic field magnitude, flow velocity magnitude (for protons), and proton number density from the Helios-1 spacecraft measurement in the inner heliosphere (at a radial distance of about 0.4 AU from the Sun) on March 3–4, 1975
Fig. 2 Magnetic field data (only the magnitude is plotted) mapped fluctuating field (Taylor’s hypothesis)

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