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Table 1.
Boundary values for solar wind parameters and turbulence quantities for the slow solar wind (SW) and fast solar wind (FW).
| Parameters | Values |
Parameters | Values |
||
|---|---|---|---|---|---|
| SW | FW | SW | FW | ||
| ⟨z∞+2⟩ (km2 s−2) | 1150 | 2180 | ⟨z*+2⟩ (km2 s−2) | 130 | 180 |
| ⟨z∞−2⟩ (km2 s−2) | 220 | 165 | ⟨z*−2⟩ (km2 s−2) | 45 | 30 |
 (km2 s−2) |
−273.4 | −400 |  (km2 s−2) |
−4.13 | −20 |
 (km3 s−2) |
4.35 ×108 | 1.24 ×109 |  (km3 s−2) |
9.83 ×107 | 6.8 ×107 |
 (km3 s−2) |
1.25 ×108 | 1.1 ×108 |  (km3 s−2) |
5.1 × 107 | 1.32 ×107 |
 (km3 s−2) |
−5.04 × 108 | −6.12 ×109 |  (km3 s−2) |
−1.52 × 107 | −5.29 ×107 |
| U (km s−1) | 345 | 490 | np (cm−3) | 15 | 15 |
| Te (K) | 3 × 104 | 5 × 104 | Tp (K) | 9.5 × 104 | 2 × 105 |
| ⟨ρ∞2⟩ (cm−6) | 4 | 1.5 | – | – | – |
Notes. The electron density is assumed approximately equal to the proton density, ne ≈ np. The proton and electron thermal pressure is determined from Pp = npkBTp and Pe = nekBTe, respectively.
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