Home › Library › Glossary › Space Environment › SAA
☀️ Space Environment

South Atlantic Anomaly (SAA)

Also known as: South Atlantic Anomaly

Quick answer

The South Atlantic Anomaly is the region over South America and the South Atlantic where the inner radiation belt sags closest to Earth, exposing low-orbiting satellites to elevated proton radiation. Instruments safe, memories flip, and operators plan around every crossing.

📘 Full definition✓ Reviewed 2026-09-07
The South Atlantic Anomaly (SAA) is the low-altitude gateway into the inner Van Allen belt: because Earth's magnetic dipole is offset from the planet's centre and tilted, field strength over the South Atlantic is anomalously weak, and the trapped proton population dips to altitudes as low as ~200 km there. Every satellite in low Earth orbit with inclination above a few degrees transits the SAA several times daily, collecting most of its total radiation dose in those minutes: single-event upsets cluster there (bit-flips in memories, latch-ups in processors), sensitive detectors — space telescopes' cameras, star trackers — record particle strikes as snowstorms of false signal, and operations respond with SAA masks: pausing science, safing high-voltage instruments, deferring critical commands until clear. The ISS's dosimeters map the anomaly in crew dose; the Hubble team's "SAA impacted" observation windows are a fixture of scheduling. The anomaly also moves — drifting westward a fraction of a degree per year and slowly deepening as the geomagnetic field weakens and reorganises, making the SAA both an engineering fact and a live geophysical observatory.
Location
South America / South Atlantic
Minimum Altitude
200 km
Cause
Weak magnetic field
Hazard
Elevated radiation for LEO sats

Understanding SAA

Designing for the daily storm

SAA fluence drives LEO radiation engineering: memory scrubbing rates are set by its upset statistics, detector designs allow for its background (some instruments simply blank), and anomaly post-mortems begin by checking the orbit position at fault time — a large share of LEO single-event anomalies geolocate straight to the SAA's footprint. Dose maps of the region, accumulated by decades of satellites, are among space physics' most practical products.

A window on the deep Earth

The anomaly is surface evidence of the geodynamo's present mood: patches of reversed magnetic flux on the core-mantle boundary beneath the South Atlantic weaken the field above, and their evolution — tracked by magnetic survey satellites — animates the SAA's drift and deepening. Whether this presages further weakening or is routine secular variation, the same maps that guide satellite operators are data for geophysicists reading the core.

See it live Watch LEO satellites transit the anomaly's footprint over the South Atlantic on the live globe. Open Live Globe →
📖 Learn More

Frequently Asked Questions

Earth's magnetic field is roughly a dipole displaced ~500 km from the planet's centre toward the western Pacific and tilted ~11°. The far side of that offset — the South Atlantic — gets the weakest field at a given altitude, and weak field lets the trapped particles mirror lower. Geometry, not geology.
Occasionally literally: crews since Apollo report light flashes — particles traversing the retina. Dose spikes during crossings dominate ISS daily totals but remain well within limits; EVA scheduling and sensitive biology experiments nonetheless keep an eye on SAA timing.
It is deepening and spreading slowly as the geomagnetic field weakens (a few percent per century) — recent models even show a developing second minimum. Changes are gradual on mission timescales, but long-lived programmes genuinely re-tune their SAA masks between generations.

Sources & References

Definitions are reviewed against primary sources. Last reviewed: 2026-09-07.