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Reconciling Parker Solar Probe Observations and Magnetohydrodynamic Theory
Tommaso Alberti et al 2022 The Astrophysical Journal Letters 940 .
Caption: Figure 4.
As in Figure 3 but separating slow (V < 400 km s−1, upper panels) and fast (V > 400 km s−1, lower panels) solar wind intervals.
© 2022. The Author(s). Published by the American Astronomical Society.
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