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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 6.

Core electron temperature Tc,e (in eV) scaled to 35.6 R, provided by the plasma QTN spectrum measured by RFS/FIELDS, against plasma speed (km s−1), provided by SWEAP/SPC. Left column: data for calm solar wind intervals only, for the entire data set (top) in state 1 (middle, red-to-black colors) in state 2 (bottom, blue-to-black colors). Right panel: same organization but for rest of the data set. Colors indicate the probability distribution function for the points.

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