Table 2.
Relative streamline angular deviation Δϕ between methods (a) and (c) and between (b) and (c) for the typical range of heliocentric distances covered by PSP (0.05–0.3 au), SolO (0.3–1 au), and Ulysses (> 1 au) based on the iso-poly ur profiles.
Ecliptic plane (θ = 0°) | |||
---|---|---|---|
ur (1 au) | < 350 km s−1 | 350–550 km s−1 | > 550 km s−1 |
|Δφ(a|c)| (PSP) | ≤3° | ≤1.5° | ≤0.5° |
|Δφ(a|c)| (SolO) | ≤4° | ≤2″ | ≤1° |
|Δφ(a|c)| (Ulysses) | ≤4° | ≤2° | ≤1° |
|Δφ(b|c)| (PSP) | 5°–18° | 1.5°–5° | ≤0.5° |
|Δφ(b|c)| (SolO) | 8″–18° | 3°–6° | ∼0.5° |
|Δφ(b|c)| (Ulysses) | 8°–18° | 3°–6° | ∼0.5° |
Polar region (θ = 60°) | |||
ur (1 au) | < 350 km s−1 | 350–550 km s−1 | > 550 km s−1 |
|Δφ(a|c)| (PSP) | 1.5°–6° | ≤2″ | ≤0.5° |
|Δφ(a|c)| (SolO) | 3°–7° | 1.5″ − 3″ | ≤1° |
|Δφ(a|c)| (Ulysses) | 2°–7° | 0.5°–3° | ≤1° |
|Δφ(b|c)| (PSP) | 4°–14° | 1.5°–4° | ≤0.5° |
|Δφ(b|c)| (SolO) | 6″–14° | 2°–4° | ∼0.5° |
|Δφ(b|c)| (Ulysses) | 6°–14° | 2°–4° | ∼0.5° |
Notes. The wind speed indicated in the table is the typical ur computed at 1 au with the iso-poly models. Deviations for a mapping at polar latitude are also computed and summarized.
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