The anomaly on the globe, 1900 to 2050
Colours: total intensity of the field at sea level (magenta = weak, blue = strong); white line: the 32,000 nT limit. Choose a year: 2050* is the extrapolated field (“extrapolated field” method), not a measurement. Light blue: the South American minimum since 1900, orange its forecast, green the African lobe and its forecast. Hover a point for its year and position.
Forecasts from 2025
| Year | South American minimum | Weakest field | Surface below 32,000 nT |
|---|---|---|---|
| 2030 | -26.2°, -61.2° (within 53 km at 90 %) | 21,919 ± 71 nT | 22.0 ± 0.1 % |
| 2035 | -26.2°, -62.4° (within 114 km at 90 %) | 21,766 ± 123 nT | 22.6 ± 0.3 % |
| 2040 | -26.0°, -63.7° (within 179 km at 90 %) | 21,614 ± 169 nT | 23.1 ± 0.4 % |
| 2050 | -26.0°, -66.3° (within 316 km at 90 %) | 21,309 ± 254 nT | 24.1 ± 0.6 % |
Intensity and extent change steadily: their forecasts are tight. The position moves slowly westwards, about 20 km a year, with errors growing beyond 20 years.
Two lobes: Africa catches up with South America
Since 2005 a second minimum exists south-west of Africa (the splitting described by Finlay et al., 2020). In 2025 it is at 23,462 nT against 22,071 nT for the South American lobe, but it weakens by about 87 nT a year against 30: if this goes on, it will become the weakest point of the Earth’s field.
| Method | 2030 : Amer. / Afr. | 2040 : Amer. / Afr. | 2050 : Amer. / Afr. | African lobe deeper in |
|---|---|---|---|---|
| extrapolated field | 21,924 / 23,022 | 21,637 / 22,137 | 21,345 / 21,245 | 2049 |
| linear trend | 21,919 / 23,025 | 21,614 / 22,151 | 21,309 / 21,278 | 2050 |
| extrapolated field with acceleration | 21,922 / 22,996 | 21,634 / 21,867 | 21,368 / 20,387 | 2043 |
The African lobe has existed for only 20 years: none of these methods could be judged on it. The spread between methods is the only measure of uncertainty, and it is large.
Show the data as a table
Show the data as a table
What the decline of the dipole explains
The dipole, the part of the field that looks like a bar magnet, weakened from 32,176 to 29,733 nT between 1900 and 2025 (-7.6 %). To measure its role, the dipole coefficients of both years are swapped, keeping the rest of the field: with the dipole of 2025 and the rest of 1900, the minimum deepens by 65 % of what it actually did; with the dipole of 1900 and the rest of 2025, by 49 %. Both effects combine (intensity is not additive). The westward drift comes entirely from the rest of the field: with the dipole of 2025 alone, the minimum would stay nearly where it was in 1900 (see the table). The anomaly is the surface trace of reversed-flux patches at the core boundary under the South Atlantic (Terra-Nova et al., 2017), which grow and move. See also the dipole moment on the pole forecast.
| Field | Weakest field | Surface below 32,000 nT | Minimum at |
|---|---|---|---|
| Actual field 1900 | 25,422 nT | 9.0 % | -22.0°, -37.0° |
| Dipole 2025, rest 1900 | 23,238 nT | 14.4 % | -21.8°, -38.7° |
| Dipole 1900, rest 2025 | 23,794 nT | 14.9 % | -25.7°, -56.5° |
| Actual field 2025 | 22,071 nT | 21.4 % | -26.2°, -60.1° |
What the methods are worth on the past
| Quantity | Method | 5 yr | 10 yr | 20 yr | Mean error 5–20 years |
|---|---|---|---|---|---|
| Position of the minimum (km) | extrapolated field | 19 / 50 | 46 / 111 | 99 / 243 | 72 |
| mean of the methods | 20 / 63 | 46 / 142 | 148 / 366 | 112 | |
| constant velocity | 18 / 67 | 40 / 184 | 99 / 362 | 83 | |
| extrapolated field with acceleration | 22 / 67 | 69 / 173 | 253 / 743 | 204 | |
| constant acceleration | 30 / 176 | 80 / 438 | 239 / 1,113 | 208 | |
| Weakest field (nT) | extrapolated field | 26 / 91 | 42 / 108 | 90 / 235 | 67 |
| linear trend | 24 / 87 | 42 / 106 | 72 / 216 | 61 | |
| mean of the methods | 28 / 97 | 51 / 162 | 133 / 407 | 107 | |
| extrapolated field with acceleration | 34 / 126 | 81 / 283 | 266 / 1,026 | 205 | |
| quadratic trend | 55 / 107 | 97 / 179 | 274 / 497 | 147 | |
| Surface below 32,000 nT (M km²) | extrapolated field | 0.4 / 0.7 | 0.7 / 1.4 | 1.1 / 2.6 | 0.87 |
| linear trend | 0.3 / 0.8 | 0.6 / 1.3 | 1.7 / 3.2 | 0.96 | |
| mean of the methods | 0.3 / 0.7 | 0.8 / 1.7 | 1.6 / 3.9 | 1.10 | |
| extrapolated field with acceleration | 0.4 / 0.9 | 1.0 / 2.8 | 3.2 / 7.6 | 2.05 | |
| quadratic trend | 0.5 / 1.0 | 0.9 / 2.1 | 2.1 / 6.6 | 1.54 |
Show the data as a table
Links with other phenomena
Dipole and poles. The anomaly grows while the dipole moment falls and the north magnetic pole runs towards Siberia (pole forecast): three aspects of one core field, not three independent causes; a correlation between these curves, all monotonic for a century, would prove nothing more. The dipole swap above gives its physical share.
Reversal? A weakening dipole and a spreading anomaly are sometimes presented as signs of a coming reversal (Pavón-Carrasco and De Santis, 2016); nothing in these data can date a reversal, which takes millennia (pole reversal).
Radiation belts. Above the anomaly the inner belt (protons) comes down to 200–800 km: that is where low-orbit satellites suffer most of their upsets (Heirtzler, 2002). Our belt measurements come from the GOES satellites, in geostationary orbit (36,000 km), where the anomaly has no effect: the link cannot be tested here, and we do not present it as measured.
Field. Total intensity F at sea level (WGS84 ellipsoid) computed every year since 1900 from the IGRF-14 Gauss coefficients (Alken et al., 2021), on a 1° grid of the sector 80° S–20° N, 130° W–70° E for the minima (position refined between nodes by parabolas) and on a 2° world grid for the surface below 32,000 nT (usual threshold, Finlay et al., 2020) and the outline. The field being linear in its coefficients, each grid is a matrix product, checked against the point-by-point computation.
Lobes. The South American lobe is the deepest minimum of 1900, followed year by year by the nearest local minimum; the African lobe starts the first year a second local minimum appears more than 2,000 km east.
Forecasts. As for the poles: velocity, acceleration, field extrapolated with its change over the last 5 years, field with secular acceleration, mean; for intensity and surface, linear (5 years) or quadratic (15 years) trend instead of velocity. Each is replayed from every year 1950–2024 at 1–25 years; the retained method has the smallest mean error at 5–20 years; the uncertainty band follows the 50 and 90 % quantiles of its past errors.
Share of the dipole. Field of the last year with the degree-1 coefficients of the first, and the reverse.
- Finlay et al. (2020)
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Finlay, C. C., Kloss, C., Olsen, N., Hammer, M. D., Tøffner-Clausen, L., Grayver, A., & Kuvshinov, A. (2020). The CHAOS-7 geomagnetic field model and observed changes in the South Atlantic Anomaly. Earth, Planets and Space, 72, 156.
· doi:10.1186/s40623-020-01252-9
Licence : Published literature; cited - Amit et al. (2021)
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Amit, H., Terra-Nova, F., Lézin, M., & Trindade, R. I. (2021). Non-monotonic growth and motion of the South Atlantic Anomaly. Earth, Planets and Space, 73, 38.
· doi:10.1186/s40623-021-01356-w
Licence : Published literature; cited - Terra-Nova et al. (2017)
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Terra-Nova, F., Amit, H., Hartmann, G. A., Trindade, R. I. F., & Pinheiro, K. J. (2017). Relating the South Atlantic Anomaly and geomagnetic flux patches. Physics of the Earth and Planetary Interiors, 266, 39–53.
· doi:10.1016/j.pepi.2017.03.002
Licence : Published literature; cited - Pavón-Carrasco et al. (2016)
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Pavón-Carrasco, F. J., & De Santis, A. (2016). The South Atlantic Anomaly: the key for a possible geomagnetic reversal. Frontiers in Earth Science, 4, 40.
· doi:10.3389/feart.2016.00040
Licence : Published literature; cited - Heirtzler (2002)
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Heirtzler, J. R. (2002). The future of the South Atlantic anomaly and implications for radiation damage in space. Journal of Atmospheric and Solar-Terrestrial Physics, 64(16), 1701–1708.
· doi:10.1016/S1364-6826(02)00120-7
Licence : Published literature; cited - Alken et al. (2021)
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Alken, P., Thébault, E., Beggan, C. D., Amit, H., Aubert, J., et al. (2021). International Geomagnetic Reference Field: the thirteenth generation. Earth, Planets and Space, 73, 49.
· doi:10.1186/s40623-020-01288-x
Licence : Published literature; cited