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Reconciling Parker Solar Probe Observations and Magnetohydrodynamic Theory

  • Authors: Tommaso Alberti, Simone Benella, Giuseppe Consolini, Mirko Stumpo, Roberto Benzi

Tommaso Alberti et al 2022 The Astrophysical Journal Letters 940 .

  • Provider: AAS Journals

Caption: Figure 1.

(From top to bottom) The plasma bulk speed V, the Alfvén speed ﹩{V}_{{\rm{A}}}=21.8\,\tfrac{B}{\sqrt{n}}﹩ (B in units of nT, n in units of cm−3), and the PSP radial distance to the Sun R. Dark and light blue lines in the top panel refer to slow (V < 400 km s−1) and fast (V > 400 km s−1) solar wind intervals, respectively.

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