Table 2.
Mean standard deviations of the tilt angles of the emerging BMRs in our model.
| Magnetic flux range [Mx] | Observed σtilt | Fitted σtilt |
|---|---|---|
| 3.0 × 1018 − 4.0 × 1020 | 107° (60.0%) | 108° (59.5%) |
| 4.0 × 1020 − 1.0 × 1023 | 46° (95.0%) | 37° (98.5%) |
| 1.0 × 1021 − 4.6 × 1021 | 30° (99.7%) | 33° (99.4%) |
| 1.0 × 1021 − 1.0 × 1023 | 25° (100%) | 28° (99.9%) |
| 4.6 × 1021 − 1.0 × 1023 | 18° (100%) | 17° (100%) |
Notes. Listed are: the magnetic flux ranges, the approximate estimates of the standard deviation derived from observations (Harvey 1993; Schunker et al. 2020, see text for details) and values returned by the best-fit approximation to these values, see Eq. (10). The values in the brackets are the percentage of regions that obey Hale’s law.
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