The South Atlantic Anomaly: The Key for a Possible Geomagnetic Reversal

• Published in: Frontiers in Earth Science
• Main Authors: Pavón-Carrasco, Fco. Javier, De Santis, A.
• Other Authors: European Space Agency, European Commission, Istituto Nazionale di Geofisica e Vulcanologia
• Format: Article in Journal/Newspaper
• Language: English
• Published: Frontiers Media 2016
• Subjects: Geomagnetism; South Atlantic anomaly; Geomagnetic reversals and excursions; Dipolar magnetic field; Harmonic analysis; South Atlantic Ocean
• Online Access: http://hdl.handle.net/10261/184585; https://doi.org/10.3389/feart.2016.00040; https://doi.org/10.13039/501100000780; https://doi.org/10.13039/501100000844; https://doi.org/10.13039/501100008034

The South Atlantic Anomaly is nowadays one of the most important features of the Earth's magnetic field. Its extent area at the Earth's surface is continuously growing since the intensity instrumental measurements are available covering part of the Southern Hemisphere and centered in South America. Several studies associate this anomaly as an indicator of an upcoming geomagnetic transition, such an excursion or reversal. In this paper we carry out a detailed study about this issue using the most recent models that also include data from the last ESA mission Swarm. Our results reveal that one of the reversed polarity patch located at the CMB under the South Atlantic Ocean is growing with a pronounced rate of −2.54·105 nT per century and with western drift. In addition, we demonstrate that the quadrupole field mainly controls this reversal patch along with the rapid decay of the dipolar field. The presence of the reversal patches at the CMB seems to be characteristic during the preparation phase of a geomagnetic transition. However, the current value of the dipolar moment (7.7 1022A·m2) is not so low when compared with recent paleomagnetic data for the Holocene (last 12 ka) and for the entire Brunhes geomagnetic normal polarity (last ~0.8 Ma), although the rate of decay is similar to that given by previous documented geomagnetic reversals or excursions. FP is grateful to the ESA-funded Project TEMPO (contract N° 4000112784/14/I-SBo, The Living Planet Fellowship) and to the postdoctoral Marie Skłodowska-Curie Individual Fellowship 659901-CLIMAGNET. AD thanks the ESA-funded Project SAFE (contract n° 4000113862/15/NL/MP-Swarm+Innovation) and the INGV-funded LAIC-U Project, for providing financial support to this research. Peer reviewed