Table 1
5-saverages and standard deviations of solar wind parameters before and after the FA mode interval.
| Parameter | Before | After |
|---|---|---|
| Vc [km s−1] | 300 ± 5.3 | 316 ± 12.1 |
| nc [cm−3] | 150 ± 16.9 | 139 ± 19.4 |
| Vc, th [km s−1] | 79.5 ± 5.7 | 69.6 ± 5.9 |
| Vb [km s−1] | 413 ± 5.3 | 428 ± 12.1 |
| nb [cm−3] | 17.8 ± 16.9 | 4.5 ± 19.4 |
| Vb, th [km s−1] | 52 ± 5.7 | 30.3 ± 5.9 |
| VA [km s−1] | 78.1 ± 5.1 | 83.1 ± 4.6 |
| T⊥∕T|| | 1.78 ± 0.3 | 1.17 ± 0.25 |
| βp|| | 0.64 ± 0.26 | 0.62 ± 0.22 |
| βp⊥ | 1.15 ± 0.24 | 0.73 ± 0.23 |
| |B| [nT] | 44.9 ± 0.25 | 44.9 ± 0.48 |
Notes. The c and b subscripts correspond to the core and beam, respectively, and the p subscript corresponds to fits of the entire proton distribution. The ratio of the proton thermal pressure (defined with respect to the background magnetic field) to magnetic pressure are denoted with β||p and β⊥p.
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