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Source-dependent Properties of Two Slow Solar Wind States

  • Authors: Léa Griton, Alexis P. Rouillard, Nicolas Poirier, Karine Issautier, Michel Moncuquet, and Rui F. Pinto

2021 The Astrophysical Journal 910 63.

  • Provider: AAS Journals

Caption: Figure 7.

Electron “flux” ne(35.6 R)Vp (in cm−2 s−1) provided by the plasma QTN spectrum measured by RFS/FIELDS and SWEAP/SPC against the square magnetic field intensity (in nT) provided by FIELDS. Left panel: data for calm solar wind interval (red for state 1, blue for state 2). Right panel: data for variable solar wind intervals (magenta for state 1, cyan for state 2).

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