Table 2.
Most probable (maximum a posteriori) parameter vector [BOLD]P, obtained after fitting the double Gaussian model described in the text to the data from E2.
| μ0ϕ | μ0θ | σ0ϕ | σ0θ |
|---|---|---|---|
 |
 |
 |
 |
| μϕ | μθ | σϕ | σθ |
 |
 |
 |
 |
| γ | |||
 |
|||
Notes. The first line presents the parameters associated with the background quiet solar wind model, the second line those associated with the switchback population, and the third line the proportion of the switchback population.
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