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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 4.

Top panel: total pressure ptot = 2nekBTc,e + pmag in black, along with the electron gas pressure pe = nekBTc,e in dark gray and magnetic pressure pmag = ∣B2/2μ0, computed with all quantities scaled to the perihelion distance of 35.6 R (see Section 2.2), all in nPa. Bottom panel: electron βe = nekBTc,e/pmag, in black for calm solar wind intervals, and in gray otherwise. Here quantities are also scaled to 35.6 R.

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