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Table 7.
Geometry of the accreting field lines derived from least squares fits to the orbital motion of the cyclotron lines (Fig. 5).
| Pole | Bsp | δf | ψf | θmin | ∠(Bsp, 1, Bsp, 2) | Δ(ϕ) |
|---|---|---|---|---|---|---|
| (MG) | (°) | (°) | (°) | (°) | ||
| 1 N | 27.2 | 36 | 49 | 45 | ||
| 2 S | 28.6 | 136 | 224 | 56 | 170.9 | 0.487 |
| 1 S | 27.3 | 126 | 57 | 46 | ||
| 2 N | 28.4 | 28 | 227 | 52 | 153.2 | 0.472 |
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