Image Details

Choose export citation format:

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 5.

Left column: data for calm solar wind intervals only, in red for state 1 and in blue for state 2. Right column: rest of the data set, in magenta for state 1 and in cyan for state 2. Top panels: electron βe scaled to 35.6 R (see Section 2.2), against proton speed in km s−1. Middle panels: electron density (cm−3) scaled to 35.6 R, against proton speed in km s−1. Error bars provided by the QTN method are plotted as thin black lines behind each point and are used to compute the error on βe. Bottom panels: magnetic field intensity (nT) scaled to 35.6 R, against proton speed in km s−1.

Other Images in This Article
Copyright and Terms & Conditions